The galaxy presents as a slightly elongated, yellowish-orange object, indicating an older stellar population. There is a smooth, diffuse quality to the light distribution, with no readily discernible spiral arm structure or distinct features. The shape is approximately elliptical but with a slight disk visible along a single plane. Hints of blue are visible on the very edges of the galaxy. The galaxy appears relatively isolated, showing no strong evidence of a major merger event. There may be some slight disturbances on the very periphery, with small, irregular light patterns, suggestive of minor interactions or tidal effects. 
