The galaxy presents as a moderately luminous, relatively compact structure. Its morphology appears to be predominantly smooth, indicative of an elliptical or lenticular galaxy type. The galaxy exhibits a slightly elongated shape. There is no apparent strong spiral arm structure or prominent dust lane. Color gradients are subtle, with a generally redder hue, suggesting an older stellar population and a potentially low star formation rate. There is no evidence of any major mergers or significant tidal disturbances in the immediate vicinity of the galaxy.
