The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. It appears elongated in shape, rather than perfectly circular. There is a discernible central bulge, exhibiting a higher concentration of light and a yellowish hue, which likely indicates a population of older stars. The outer regions of the galaxy fade gradually into the background, displaying a bluer tint, suggesting a possible presence of younger stars and ongoing, but perhaps modest, star formation activity. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy does not show any obvious signs of recent major merger activity or significant tidal disturbances.
