The galaxy appears to be a relatively compact object, with a predominantly smooth morphology. It exhibits a slightly elongated shape, deviating marginally from a perfectly circular form. The central region displays a bright, concentrated luminosity, possibly indicative of an active galactic nucleus or a dense stellar population. Moving outwards from the center, the light gradually diffuses, with a faint, extended halo surrounding the core. There is subtle evidence of a possible minor disturbance or interaction, suggested by a slight asymmetry in the outer regions of the galaxy. The overall color profile suggests a population of older stars, although subtle color variations imply there may be ongoing, but relatively low, star formation activity within the galaxy.
