The galaxy appears to be a relatively compact object, exhibiting a largely smooth morphology, but with some notable features. It is observed to be generally round in shape, with a somewhat concentrated central region. The color profile suggests a range of stellar populations, with a brighter, bluer core and a more yellow-red halo, indicating older stars away from the core. Possible indication of disturbance or star formation activity is observed in the region surrounding the galaxy, though is faint. There is no clear indication of a prominent disk structure, and the system is not visibly undergoing a major merging event.
