The galaxy presents a somewhat smooth, rounded morphology, but there is some indication of a subtle disk-like feature. The light distribution suggests a central bulge, with a gradual decrease in luminosity outwards. There is some asymmetry in the distribution of the outer regions, possibly indicating some past or ongoing minor disturbance or interaction. The galaxy exhibits an overall yellowish hue suggesting an older stellar population and a relatively low rate of star formation. The size appears moderate, indicating a galaxy of substantial, but not exceptionally large, physical extent. There is no strong visual evidence of a major ongoing merger or significant tidal features.
