The galaxy presents as a centrally concentrated object with a notable elliptical morphology. Its core exhibits high luminosity, appearing nearly spherical. Diffuse light extends from the central region, gradually fading into the background sky. The overall color profile is slightly redder than expected, suggesting either an older stellar population or significant dust obscuration. There is a subtle hint of asymmetry in the outer regions, possibly indicative of past or ongoing interactions. No distinct spiral arm structures or prominent star-forming regions are readily discernible in this image. The galaxy appears relatively smooth, suggesting a lack of significant recent merger activity.
