The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population and potentially a lower rate of on-going star formation. The galaxy lacks prominent spiral arm features or well-defined dust lanes, indicating a more quiescent morphology. It shows an overall elongated shape, appearing more 'in between' round and cigar-shaped and not perfectly spherical. There is no obvious sign of major mergers, or tidal disturbances. A faint disk is potentially present but is not well defined. The galaxy appears to be relatively isolated.
