This galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. There is a noticeable color gradient, exhibiting a yellowish-white core that transitions to a redder hue in the outer regions. The galaxy lacks any clear spiral arm structure or prominent dust lanes. There is no evidence of major mergers or significant tidal disturbances. Based on its overall appearance and color profile, this galaxy likely has a low star formation rate and may be dominated by an older stellar population.
