The galaxy presents a generally elliptical morphology, with a smooth appearance and no readily discernible spiral arm structure. A bright, concentrated central bulge dominates the galaxy's luminosity profile, with a notable decrease in surface brightness towards the outer regions. Color gradients are subtle, with a yellowish hue concentrated in the bulge, possibly indicating an older stellar population. The outskirts exhibit a slightly bluer tint, potentially suggesting more recent star formation, although this is not definitively evidenced by discrete star-forming regions. The galaxy appears relatively isolated, showing no strong signs of tidal interactions or ongoing mergers in the immediate vicinity, although there may be very minor distortions. Based on the apparent size and overall luminosity, this galaxy is likely a moderately massive system.
