The galaxy presents as a largely smooth, centrally concentrated object. Its overall shape appears roughly elliptical, exhibiting minimal disk-like features. The color profile indicates a relatively homogeneous distribution of older stellar populations. While the galaxy appears largely undisturbed, there may be faint indications of minor tidal features, such as faint light extending from the central body. Star formation appears to be largely quiescent, with the dominant light stemming from evolved stars. There is a noticeable lack of prominent spiral arms or distinct dust lanes. The central bulge dominates the overall morphology, suggesting a considerable mass concentration at the galaxy's core. The galaxy appears to be relatively isolated, showing little interaction with nearby galaxies in this field of view.
