The galaxy presents a predominantly smooth appearance, indicative of a relatively evolved system. A faint, disc-like structure is suggested by the slightly elongated morphology, though not strongly defined. The overall colour profile suggests a mix of stellar populations, with a central yellowish-white concentration potentially indicating an older, more established population. The apparent size is relatively small, which could be an indication of the galaxy's intrinsic properties or its distance. There is no clear evidence of ongoing major mergers, although subtle irregularities in the galaxy's shape might indicate minor disturbances.
