This galaxy appears to be relatively compact, exhibiting a concentrated light profile. The object presents with a dominant central bulge or core. Evidence suggests it might be undergoing minor interaction or disturbance, marked by slight asymmetries in its overall structure. The color index indicates an increased redder color, suggesting a substantial population of older stars or dust obscuration. The majority of the object's light is concentrated within a radius that would be considered moderate for a galaxy of its apparent brightness. Observed features are subtle, but hint at a possibility of ongoing or past minor merging activity.
