The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is no prominent spiral structure or bar visible. The light distribution is consistent with an elliptical or lenticular galaxy, though a disk cannot be entirely ruled out at this resolution.

The galaxy exhibits a moderate color gradient, with a slightly bluer hue towards the outer regions and a more yellow/red color near its core. This may indicate ongoing star formation in the outer regions. There is no apparent dust lane obscuring the light.

Based on the overall appearance, this galaxy could be classified as an early-type galaxy. There is evidence of minor disturbances or interactions, but it's not very pronounced.
