The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The overall shape is elongated, exhibiting a cigar-like appearance. The core region displays a distinct yellowish-orange hue, suggestive of an older stellar population. The outer regions fade into a bluer color, which may indicate some active, but limited, star formation. There appears to be a slight asymmetry, suggesting possible interactions, though the overall structure appears undisturbed. There is no clear evidence of spiral arms or a well-defined disk structure.
