The galaxy presents as a substantial, resolved object with a dominant central bulge. The color profile suggests a population of older stars within the bulge, exhibiting a reddish-yellow hue. The overall structure appears relatively smooth, with a notable absence of distinct spiral arms or prominent dust lanes. There may be some minor disturbances in the outer regions, as hinted by the asymmetry in the distribution of light around the main body. The galaxy displays an extended halo or envelope surrounding the core, gradually fading into the background sky. While the galaxy seems largely isolated, there are suggestions of potential minor interaction or past mergers, as indicated by the slight irregularities in its morphology. Overall, the galaxy appears to be a massive, evolved system, possibly an early-type spiral galaxy.
