The galaxy presents as a somewhat elliptical, smoothly distributed light source. A pronounced central bulge is observed, exhibiting a concentrated luminosity. The color gradient transitions from a slightly yellower hue in the central region to a marginally bluer tint towards the outer edges, suggesting a potentially older stellar population concentrated in the bulge with hints of younger stars toward the periphery. The overall structure suggests a likely early-type galaxy, possibly of type S0. No distinct spiral arms or significant dust lanes are discernible within the available imagery, indicating a relatively quiescent star formation rate. There is no apparent evidence of ongoing merger activity or significant tidal disturbances affecting its morphology.
