The galaxy appears to be a relatively small, faint, and somewhat irregular object. It is roughly circular in overall appearance, but lacks a well-defined structure.  The central region exhibits a slightly brighter luminosity, suggesting a weak galactic nucleus or a concentration of older stars. 

There are some subtle irregularities in the outer regions, potentially indicative of minor gravitational disturbances or recent interactions with other galaxies. It is plausible that there are faint tidal features or evidence of past mergers, but these are not clearly defined. The color profile suggests a mix of stellar populations.
