The galaxy presents a generally smooth morphology, appearing somewhat elliptical in shape, although not perfectly round. The light distribution is concentrated towards the center, indicating a significant bulge component. The color profile suggests a mix of stellar populations. The central region exhibits a bluer hue, potentially indicative of ongoing star formation within a spiral disk of the galaxy, while the outer regions appear redder, implying an older stellar population. There is no clear sign of spiral arms or a bar structure. The galaxy shows some minor signs of gravitational disturbance, it is interacting and possibly merging with a smaller dwarf galaxy which is seen close by. The overall impression is of a moderately massive galaxy, potentially undergoing some recent star formation activity in its disk that could be caused by the smaller merging galaxy.
