The galaxy appears as a moderately bright, centrally concentrated object. It presents a smooth, elliptical morphology, exhibiting a high degree of radial symmetry. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a primarily bulge-dominated system. The color appears relatively uniform across the galaxy, leaning toward a slightly redder hue, which could be indicative of an older stellar population. There may be some minor disturbances or irregularities present in the light profile, but these do not appear to be major merger events. Overall, the galaxy seems to be an early-type galaxy, likely an elliptical or lenticular galaxy, with a relatively quiescent star formation history. Its physical size appears small.
