This galaxy exhibits a largely smooth morphology, appearing mostly round in shape. The central region presents a bright, concentrated luminosity, suggesting a substantial stellar population or the presence of an active galactic nucleus. A gradual decline in surface brightness extends outwards from the core, indicative of a spheroidal or elliptical structure. There is very little evidence of spiral arms or significant dust lanes. The galaxy exhibits a redder hue compared to typical spiral galaxies. There are no indications of tidal features or ongoing major mergers, although some minor asymmetry may be present. The overall characteristics suggest a relatively evolved system with a suppressed star formation rate.
