The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards a bright central core, indicating a likely bulge structure with a high degree of sphericity. The galaxy appears to be relatively undisturbed, with no obvious signs of recent major mergers or tidal interactions. There may be hints of a very faint, diffuse disk component or spiral arms, but it is difficult to tell. The galaxy color profile displays a redder hue, suggesting a relatively older stellar population with suppressed star formation.
