The galaxy presents as a centrally concentrated object. The overall color profile suggests a relatively evolved stellar population, exhibiting a yellowish hue, possibly indicative of older stars and a lower rate of active star formation. The galaxy's shape is generally round. There is no clear evidence of significant spiral arm structure or a prominent disk. There is no obvious signs of ongoing major mergers or strong tidal disturbances. The galaxy shows signs of a small degree of asymmetry, suggesting the possibility of a recent, minor interaction or internal dynamical processes. Overall, the galaxy appears to be a relatively massive, quiescent system with a smooth morphology.
