The galaxy presents as a relatively smooth, elongated structure, likely an elliptical or lenticular galaxy seen at an angle. There is a concentration of light toward the galaxy's center, suggesting a prominent galactic bulge. A faint disk is potentially present, but difficult to confirm given the viewing angle and limited resolution. The color profile of the galaxy appears yellowish-white, indicative of an older stellar population. There is a possibility of minor gravitational disturbance on the edges, however, that cannot be confirmed. There is no strong evidence of significant star formation activity based on the color profile. Overall, the galaxy seems to be a mature system without substantial ongoing star formation.
