The galaxy presents as a somewhat elliptical structure. There is a prominent central bulge that appears yellowish in color, indicative of an older stellar population. The galaxy displays a disk, but it appears patchy and disturbed. Faint spiral arm structures can be inferred within the disk. Some blueish regions within the disk suggest active star formation is occurring. The galaxy's overall light distribution appears relatively smooth, with the bulge dominating the visual appearance. The galaxy exhibits an overall reddish hue, potentially signifying a substantial amount of dust obscuration or a higher proportion of older stars. The presence of disturbed features and a possible merging event indicates the galaxy is likely undergoing interaction with another galaxy.
