The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally round morphology, with a very slight elongation that does not significantly deviate from a circular shape. The light distribution suggests a centrally concentrated brightness profile, with a gradual decrease in luminosity moving outward from the core. Color gradients are subtle, displaying a reddish-yellow hue in the central region, which may indicate an older stellar population. There is no obvious evidence of spiral arms, a well-defined disk, or ongoing major merging activity. Minor asymmetries or disturbances may be present upon closer inspection, but they do not dominate the galaxy's overall structure. The galaxy’s considerable distance contributes to its small angular size.
