The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears centrally dominated, with a gradual decline in surface brightness moving outward from the core. There is a general lack of distinct spiral arm features or prominent dust lanes. The overall color suggests an older stellar population, with a yellow-red hue indicative of evolved stars. There might be a hint of a faint, extended halo surrounding the central region, but this is difficult to discern with certainty. There does not seem to be any evidence of ongoing major merging activity or significant tidal disturbances. The galaxy appears relatively undisturbed, suggesting that it's a passively evolving system.
