The galaxy appears as a moderately bright object with a slightly irregular morphology. Its overall shape seems to be somewhat elongated, rather than perfectly circular, tending toward an elliptical classification. There is evidence of a possible disk structure but it is faint. Patches of varying intensity suggest underlying features. 

Color gradients are subtle, hinting at a complex stellar population, potentially with regions of both younger, bluer stars and older, redder stars. There are some indications of possible minor disturbances within the galaxy's structure, with subtle asymmetries and faint tidal features. There is also some merging activity. There are hints of blue star forming regions, and redder, dustier areas.
