The galaxy presents a slightly elongated, though predominantly round, overall form. It is characterized by a bright, concentrated central bulge that dominates its morphology. This bulge appears relatively smooth and featureless.

Surrounding the bulge is a fainter, more diffuse halo. The outer regions of the galaxy show some irregular features, potentially indicating ongoing interactions or past merger events. There are some possible signs of tidal tails or disrupted structures extending from the main body.

The color profile suggests a stellar population that is dominated by older stars, particularly in the central bulge, indicating a low level of ongoing star formation activity. The halo appears slightly bluer, suggesting the presence of some younger stars.

There is evidence of a complex structure, indicative of potential disturbances. The overall impression is that this galaxy is in a state of transition, possibly influenced by mergers or interactions with other galaxies in its environment.
