The galaxy presents a generally smooth appearance, with a dominant central bulge. It has a somewhat elongated, cigar-like shape, suggesting it could be an elliptical galaxy or a spiral galaxy viewed at an oblique angle. The central region appears to have a higher concentration of older stars, indicated by the yellowish-orange color. There's evidence of a fainter, bluer disk or extended structure surrounding the bulge, suggesting the presence of younger stars and possible ongoing star formation, though at a relatively low rate. No signs of major mergers or tidal disturbances are visible. The galaxy does not exhibit strong spiral arm features.
