The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification. The overall shape is elongated, with an aspect ratio indicating a cigar-like appearance. A bright central bulge is clearly visible, indicating a high concentration of older stellar populations. The galaxy exhibits a gradual color gradient from the center outwards, with the core appearing more yellow, transitioning to a bluer hue in the outer regions. There is no discernible spiral structure or distinct dust lanes, consistent with a relatively quiescent star formation rate. The galaxy appears relatively isolated, showing no strong signs of recent or ongoing mergers or tidal interactions, although some minor irregularities in the outer regions cannot be ruled out completely. The apparent size is small, suggesting considerable distance.
