The galaxy presents as a centrally concentrated object, characterized by a high degree of smoothness. The morphology appears largely elliptical, exhibiting a nearly circular shape. There is no discernible disk structure or spiral arm features. The color profile indicates a relatively red population, with a significant fraction of older stars likely contributing to the overall luminosity. No signs of ongoing major merging events or tidal disturbances are evident, although subtle features indicative of minor gravitational interactions cannot be entirely ruled out. The observed size suggests a galaxy of moderate spatial extent, with an estimated stellar mass range of 10^10 solar masses. The rate of star formation appears comparatively low, which is consistent with a galaxy dominated by an older stellar population and exhibiting suppressed ongoing star formation. Overall, the galaxy appears to be a relatively quiescent, evolved system.
