The galaxy presents as a single, moderately concentrated light source with a slightly elongated morphology. The light distribution appears relatively smooth, without significant features or spiral arm structures immediately apparent. The color is primarily yellowish, indicating a possible older stellar population, with a subtle reddish hue in the central region. There is a slight asymmetry in the outer isophotes, possibly suggesting a minor tidal disturbance or interaction with another galaxy. The overall appearance indicates that this galaxy may be an elliptical or lenticular type, with a relatively quiescent star formation rate. However, the slight asymmetry warrants further investigation to determine if it is undergoing a merging process.
