The galaxy presents as a relatively small, elliptical structure. The central region exhibits a bright, concentrated core, gradually fading into a diffuse halo. Its overall form appears smooth, lacking any distinct spiral arms or prominent dust lanes, suggesting an older stellar population. The galaxy's shape tends toward an intermediate elliptical, being neither perfectly spherical nor highly elongated. There is no indication of any ongoing major merger events or significant tidal disturbances affecting its structure, though there is a possible very slight asymmetry. The color profile seems relatively uniform across the galaxy, displaying a general overall bluish white hue, indicating at least some ongoing active star formation.
