The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical or lenticular type. The light distribution appears centrally concentrated, with a bright nucleus that diminishes outwards. There is little evidence of spiral arms or prominent dust lanes. The color profile shows a tendency towards redder hues, possibly indicating an older stellar population. A slight elongation is visible in the overall shape but no major disturbances in the structure can be identified, perhaps some faint structures near the outer region of the galaxy. Indications suggest that star formation is low.
