The galaxy presents a generally smooth morphology, with an elongated, cigar-shaped appearance. Its central region displays a prominent concentration of light, appearing yellowish-white in color, suggestive of an older stellar population. Moving outward from the core, the galaxy exhibits a gradual decrease in luminosity. Fainter, bluish hues are visible in the outer regions of the galaxy, potentially indicating the presence of younger, hotter stars or regions of ongoing star formation. There is no strong evidence of spiral arm structure or distinct features, rather a more amorphous shape. Subtle irregularities or minor disturbances are suggested by slight asymmetries in the light distribution; however, major distortions or merging activity are not apparent in the image. The overall impression is of an elliptical or lenticular galaxy, possibly at a moderate distance. The estimated size appears small but the galaxy has an appreciable luminosity.
