This galaxy exhibits a generally smooth morphology, appearing as an elliptical or lenticular type when observed in the optical wavelengths presented. The object demonstrates a centrally concentrated luminosity profile, with light intensity gradually decreasing from the core towards the outer edges. The overall shape is somewhat elongated but not excessively so. There is a subtle color gradient; the central region presents a yellowish hue, potentially indicating an older stellar population, while the outer regions are a bit redder in comparison. This color difference could be due to the distribution of stars with differing ages and metallicities. No prominent spiral arms, distinct dust lanes, or signs of active star formation regions are obviously visible upon observation. There is no evidence of any major merger events, tidal tails, or distortions to the overall shape. The galaxy appears relatively undisturbed.
