The galaxy presents as a moderately bright, elliptical-like system. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. The overall shape is somewhat amorphous, lacking well-defined spiral arms or a distinct disk structure. Faint blue tinges are visible in the outer regions, hinting at the presence of some younger, hotter stars and possibly ongoing star formation, though at a relatively low rate. There are some asymmetries or subtle disturbances in its morphology. The object appears relatively isolated, with no obvious signs of a major merger event. The galaxy is somewhat diffuse, with no particularly prominent knots or regions of intense star formation visible in this image.
