The galaxy presents as a moderately luminous object, exhibiting a somewhat elongated, cigar-shaped morphology. The central region displays a brighter, concentrated luminosity profile, suggesting a substantial stellar population and potentially an active galactic nucleus. There is a hint of a second, less luminous object near the galaxy. The color distribution leans towards the redder end of the spectrum, indicating a significant population of older stars and potentially elevated dust content. Evidences of a disk are not clearly visible. There is a potential interaction with another galaxy.

