The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge. The color profile suggests a population of older stars, with a tendency towards redder hues throughout the galaxy's body. The galaxy appears to be mostly undisturbed, without significant tidal tails or indications of recent major mergers. There is a slight asymmetry to the outer isophotes, hinting at a possible minor interaction in the distant past. Star formation activity appears suppressed, aligning with the redder color indices and smooth morphology. Overall, this galaxy appears to be a mature system with little ongoing star formation and a settled structure.
