The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a high degree of radial symmetry. The central bulge is prominent and bright, with a concentrated light profile. The color indices suggest a relatively red color, indicative of an older stellar population with less ongoing star formation. There is a noticeable absence of distinct spiral arms or prominent dust lanes. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, exhibiting a well-defined, undisturbed structure. Overall, the morphology is consistent with an early-type galaxy, likely a passively evolving system.
