The galaxy appears as a centrally concentrated object with a generally smooth morphology. The central region exhibits a bright, somewhat diffuse glow, indicative of a concentrated stellar population. Faint, extended features are visible around the central bulge, giving the impression of a more extended halo or disk-like structure although no defined spiral arm structure is visible. There's a hint of some possible minor disturbances within the immediate vicinity of the object, but it otherwise shows no distinct signs of major ongoing merger activity. The overall color suggests that the stellar population is likely dominated by older stars, with possibly moderate levels of recent or ongoing star formation activity. The object displays a generally rounded appearance although with some deviation from perfect circular symmetry.
