The galaxy presents as a moderately sized, relatively luminous object with a discernible but somewhat irregular shape. There is evidence of a galactic disk structure, though it appears disturbed or undergoing an interaction. The central bulge is visible as a brighter, more concentrated region, which suggests the presence of an older stellar population. The galaxy appears to be composed primarily of older stars and gas. There may be ongoing star formation, as there is some evidence of bluer regions, but the overall star formation rate is generally low, and the color is dominated by redder, more evolved stars. The presence of tidal features are indicative of recent or ongoing gravitational interaction with another galaxy. There is a high likelihood that this galaxy is a merger remnant or in the process of merging with another galaxy.
