The galaxy presents a primarily smooth morphology, with a notable central bulge exhibiting a slightly brighter, concentrated light profile. The overall shape appears to be somewhere between round and elliptical, with the suggestion of a disk component contributing a subtle flattening. There are no obvious signs of spiral arm structure or significant dust lanes visible in this image. The color profile indicates a higher concentration of older stellar populations, particularly within the central regions, as evidenced by the redder hues observed there. No signs of ongoing major merger activity or tidal distortions are readily apparent; if present, any such interactions appear to be subtle or in an early stage. The light output from the galaxy indicates it is a galaxy with medium luminosity. Given its characteristics, this galaxy appears to be a relatively evolved system.
