The galaxy appears as a smooth, luminous object, exhibiting an elliptical morphology. It possesses a concentrated central bulge, characterized by a yellowish-white hue, indicating an older stellar population. There is very little evidence of spiral arm structure or dust lanes. The galaxy's overall shape is predominantly round. A small satellite galaxy can be seen to the right of the primary galaxy. There is no obvious strong evidence of on-going major merging activity or significant tidal disturbances.