The galaxy presents as a somewhat elliptical structure with a bright, concentrated central bulge. The light profile appears relatively smooth. Faint extensions are visible extending outwards from the central region, particularly towards the upper left direction of the frame. There appears to be a slight asymmetry, possibly indicating some form of gravitational disturbance or past interaction. The color gradient suggests a relatively old stellar population within the bulge, while the outer regions may contain younger, bluer stars. Evidence of ongoing, albeit relatively low, star formation is plausible. There is no prominent spiral structure evident, although faint hints of a disk-like morphology are possible within the noise. The galaxy does not appear to be a strong merger candidate, although the slight asymmetry points to a possible minor interaction in the past.
