The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears elliptical. The color profile indicates a dominant older stellar population, with a yellowish hue more pronounced toward the core. There is a suggestion of a slight radial color gradient, with the outer regions exhibiting a subtly bluer tint compared to the nucleus, but the difference is minimal. No distinct spiral arms or prominent dust lanes are discernible. There are no obvious signs of on-going major mergers or significant tidal disturbances. The galaxy's symmetrical appearance, coupled with the lack of prominent features, implies it is likely a relatively relaxed system.
