The galaxy presents as a relatively compact and elliptical system. Its overall form appears smooth and spheroidal, with a concentrated central bulge region exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions of the galaxy display a gradual fading in brightness, with a more diffuse and slightly bluer color, suggesting the presence of some younger stars or ongoing star formation, although limited. There is no clear indication of spiral arms or a well-defined disk structure. The galaxy appears undisturbed, showing no obvious signs of tidal interactions or major mergers.
