The galaxy presents an overall elliptical morphology, appearing somewhat elongated. The light distribution suggests a smooth profile, lacking prominent spiral arms or distinct features. The central region exhibits a higher concentration of light, indicative of a possible bulge component. The overall color appears slightly redder, which could indicate an older stellar population and/or the presence of dust obscuration. Faint diffuse emission extends outwards, suggesting the presence of a halo or extended stellar envelope. There is a small bright spot to the upper left that may be an interaction. The galaxy does not appear to be undergoing any major merging events.