The galaxy presents a flattened, elongated morphology, resembling a cigar shape when observed from this angle. Its primary axis extends significantly beyond the minor axis, suggesting a disk-like structure viewed at a high inclination. The central region exhibits a concentrated, bright nucleus, indicative of a dense stellar population or possible active galactic nucleus. The light from the galaxy appears relatively smooth, with no prominent spiral arms or distinct dust lanes visible. The galaxy's overall color profile suggests a population of older stars, with a bias toward redder wavelengths, although there may be some younger, bluer stars present. There is minimal evidence of ongoing major mergers or significant tidal disturbances, although there may be minor distortions indicating past interactions. The overall visual impression is of a relatively quiescent galaxy that has undergone a period of stellar formation in the past, but is now in a later stage of its evolution.