The galaxy presents a largely smooth morphology with a concentrated central bulge that displays a distinct bright, luminous core.  The overall shape appears to be elliptical or lenticular, exhibiting a generally rounded structure though perhaps tending towards a slightly elongated form. There is no clear indication of spiral arms or a well-defined disk. The color gradient suggests an older stellar population, with the central region appearing bluer, but quickly fading into a more red population. The galaxy is relatively compact, with a concentrated stellar distribution. The outer regions show a gradual decrease in surface brightness, with no sharp edges or truncation observed. There is no evidence of significant tidal disturbances or ongoing major mergers. Overall, this galaxy appears to be a relatively isolated, evolved system with minimal recent star formation.
