The galaxy presents an overall elliptical morphology, with an elongated, cigar-like shape. The light distribution appears relatively smooth, indicating a lack of prominent spiral arm structures. The central region exhibits a concentration of light, suggesting a central bulge or nucleus. The galaxy displays a color gradient, with the core appearing more yellow/orange, potentially indicating an older stellar population, while the outer regions seem bluer, possibly associated with younger stars or ongoing star formation. There appears to be a faint disk present, viewed edge on. There is no visual evidence of major mergers or significant tidal disturbances; however, slight disturbances cannot be ruled out. The galaxy exhibits a moderate level of intrinsic luminosity.
