The galaxy presents as a slightly elongated, lenticular-shaped structure. The central bulge appears luminous and exhibits a yellow-white hue, suggesting a population of older stars. The surrounding disk is less prominent, displaying a smoother texture with hints of blue-green coloration, potentially indicative of some younger stellar populations and ongoing, though diminished, star formation activity. No distinct spiral arm structures are readily discernible. The overall morphology suggests the galaxy is in a relatively evolved state. There is potential evidence of some minor tidal disturbances or interactions visible as faint asymmetric features extending from the main body.
