The galaxy presents as an elliptical morphology, exhibiting a generally smooth appearance. The core region displays a concentrated and bright luminosity, suggesting a high density of stars and possibly an active galactic nucleus, though further spectral analysis would be needed to confirm this. The overall shape is elongated, approximating a cigar shape, with a slight asymmetry. The color gradient appears to shift from a predominantly yellow/orange hue in the central bulge, subtly transitioning to redder tones within the outer halo. There are no obvious spiral arm structures or dust lanes visible, and there is no evidence of a strong ongoing merging event or major tidal disruptions. A slight visual distortion could be interpreted as minor disturbance.
