The galaxy presents as a centrally concentrated object with a generally smooth morphology. The light distribution appears centrally condensed, indicative of a prominent bulge component. The overall shape appears more elliptical than spiral, though there is potentially a faint, diffuse disc extending beyond the bright central region. There is little visible evidence of spiral arms or bar structures. The color profile suggests a redder core, potentially indicative of an older stellar population and dust obscuration. There are hints of bluer light in the outer regions of the galaxy, perhaps indicating more recent, although limited, star formation activity. There are no obvious signs of interaction or tidal features, suggesting this galaxy is relatively undisturbed. There are no visible signs of an active galactic nucleus.
