The galaxy presents as a moderately luminous object with an elliptical morphology. Its color profile exhibits a central concentration of yellow light, suggesting an older stellar population likely dominated by red giants and/or a significant bulge component. The outer regions display a fainter, slightly bluer hue, potentially indicating ongoing, though subdued, star formation or the presence of a younger stellar population in the disk. 

There appears to be some disruption present on the left side of the galaxy, in the form of a faint tidal tail. This could be due to an interaction with another galaxy.
