The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a high degree of central concentration, with the majority of its light emanating from a bright, well-defined core. The isophotes appear to be generally elliptical in shape, with a flattening ratio of approximately 0.85. There is no obvious evidence of spiral arm structure or significant dust lanes. The color appears consistent throughout the galaxy, with a moderate reddish hue. The overall impression is that of a mature galaxy, likely dominated by an older stellar population. No signs of on-going major mergers or significant tidal disturbances are visible.
