The galaxy presents as a slightly elongated, relatively smooth structure. It exhibits a concentrated central bulge with a yellowish hue, suggesting an older stellar population. There is a hint of a disk component, though it is not well-defined, appearing somewhat amorphous and less luminous compared to the central bulge. A subtle, elongated feature extends from one side of the central bulge, potentially indicating tidal interactions or a minor disturbance. Overall, the galaxy appears to be relatively isolated with little to no star formation observed.