The galaxy presents as an elongated, cigar-shaped structure with a relatively smooth appearance. It exhibits a concentrated central bulge region that appears yellowish-orange in color, suggesting a higher concentration of older stars. The outer regions of the galaxy appear somewhat fainter with a bluer tinge, possibly indicating the presence of a younger stellar population and ongoing, albeit low levels of star formation. There is little to no evidence of spiral arm structure or significant dust lanes. There is some evidence of minor tidal disturbances in the form of a very faint extension. Overall, the galaxy appears to be an elliptical galaxy, possibly undergoing a minor merger.
