The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is prominent and displays a yellowish hue, suggestive of an older stellar population. Moving outward from the bulge, a faint disk component becomes apparent, exhibiting a bluer color, possibly indicating some recent star formation activity, although subdued. The galaxy has a generally rounded morphology, showing no significant signs of tidal disturbances or ongoing major mergers. There may be a minor perturbation or faint feature at one location, but it does not significantly disrupt the overall structure. The galaxy appears to be relatively isolated, without a strong indication of interaction with nearby companions. Overall, the galaxy is dominated by an older stellar population and a smooth, regular structure, with minimal evidence of recent, intense star formation.
