The galaxy presents as a centrally concentrated, largely spheroidal object. There is little evidence of significant disk structure. The light profile appears smooth and diffuse, suggesting a relatively old stellar population. Some faint blue light is visible, which may indicate some present star formation. There are hints of minor asymmetry or disturbances in the outer regions, possibly indicative of a past or ongoing minor interaction or accretion event. The galaxy appears isolated, with no nearby companions that would suggest a major ongoing merger.
