The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform across the galaxy, suggesting a lack of prominent spiral arms or distinct substructures. The galaxy exhibits a yellowish hue, which could indicate an older stellar population and a relatively low rate of on-going star formation. The overall shape is elongated, though tending towards round, and there is no evidence of significant tidal distortions or ongoing merger activity. The galaxy appears to be a relatively undisturbed system.
