The galaxy presents as a smooth, elongated structure, suggesting an elliptical morphology. The galaxy exhibits a distinct cigar shape. The light distribution appears concentrated towards the center, indicating a dense core. There is a general lack of distinct features such as spiral arms or prominent dust lanes. The overall color profile seems relatively uniform, with a slight reddish hue, possibly indicating an older stellar population. There is no evidence of ongoing major merging activity or significant tidal disturbances in its immediate vicinity.
