The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a pronounced central bulge that appears bright and concentrated. Moving outwards from the core, the luminosity gradually decreases, showing a diffuse halo surrounding the central region. The galaxy appears to be more elongated than circular, suggesting a classification toward the elliptical side on the Hubble sequence. The color profile shows a yellow-orange hue, implying a population of older stars, with a possibility of low levels of on-going star formation. There is no visual evidence of spiral arm structure or significant dust lanes. The overall impression is that of a well-evolved galaxy that has largely ceased significant star formation activity. There does not seem to be any major distortion to the object, with only minimal signs of possible disturbances.