The galaxy presents as an elliptical morphology, with a relatively smooth light distribution and no readily apparent spiral arm structures. There is a slight elongation in its overall shape. The central region exhibits a brighter, more concentrated light intensity, indicating a nucleus or bulge. The color appears somewhat redder overall, implying an older stellar population or the presence of dust obscuration. There are some indications of possible tidal disturbances or a past merger event in the outer regions of the galaxy, based on the faint, disturbed light distribution.
