The galaxy presents as a singular, relatively symmetrical object with a smooth, concentrated luminosity profile. The core exhibits a bright, somewhat diffuse glow that fades gradually towards the outer regions. No distinct spiral arms or bar structures are discernible within the resolution afforded by the image. The overall color appears to be predominantly yellow, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no immediately visible indication of tidal distortions or other signs of recent merger activity. The morphological classification indicates that this galaxy is most likely a smooth elliptical or a lenticular type.
