The galaxy presents a generally smooth morphology, exhibiting a central bulge that dominates the overall light profile. The bulge appears relatively bright and concentrated. The galaxy’s shape is somewhere between round and elongated, more towards the in between end, without a clear spiral structure or bar visible. There may be a faint, diffuse disk component surrounding the bulge, but its presence is not definitively discernible in this image. The color suggests a population of older stars, possibly with ongoing but not very active star formation. There are no obvious signs of a major merger or significant tidal disturbances, though minor disturbances can not be entirely ruled out.
