The galaxy appears to be a relatively smooth, elliptical galaxy, with a concentrated central bulge. There is little to no visible dust or spiral arm structure. The color gradient suggests a higher concentration of younger, bluer stars in the central regions, transitioning to redder, older populations towards the outskirts. It exhibits a moderately compact morphology, with a projected effective radius on the order of a few kiloparsecs. There's no visual evidence of significant tidal disturbances or ongoing major mergers. A slight asymmetry could suggest a minor interaction in its past. Overall, this galaxy presents as a fairly evolved system, potentially undergoing continued, low-level star formation activity.
