The galaxy presents a complex morphology, exhibiting characteristics of both a smooth elliptical system and a disturbed disk galaxy. It shows a distinct color gradient. A bright, redder region dominates one end of the galaxy, and a bluer area is present closer to the center, possibly indicating the presence of younger stellar populations or regions of active star formation within that area. 

A plume-like extension emanates from the bluer region. This structure could be a tidal tail resulting from a gravitational interaction with another galaxy, or a remnant of a previous merger. Further investigation is needed to ascertain the precise cause.

The galaxy does not appear perfectly symmetrical, and appears to have some significant irregularities in its overall light distribution. This suggests the possibility of ongoing or recent merger activity. There is no obvious spiral arm structure visible, but there seems to be a faint disk-like structure embedded within the galaxy. Further data in different wavelengths may reveal more detailed features obscured in this visual band image.
