The galaxy presents as a relatively small, elongated object with a noticeable disk structure. The primary color of the galaxy is a warm yellowish-orange, suggesting a dominant population of older stars. There are hints of bluer regions, potentially indicating areas of more recent star formation. The galaxy appears generally undisturbed, with no obvious signs of major mergers or tidal interactions. The disk is noticeably elongated, suggesting a classification as a possible spiral galaxy viewed nearly edge-on.
