The galaxy presents as an elongated, cigar-shaped structure. Its color profile suggests an older stellar population, indicated by the reddish-yellow hue dominating the central and outer regions. There is a smooth, blended texture to its light distribution across the disk, lacking prominent spiral arm structures or distinct knots of star formation. The apparent smoothness and color are consistent with an elliptical galaxy, or potentially a lenticular galaxy viewed at a high inclination. There are no clear signs of an ongoing major merger or tidal disturbances. The galaxy appears relatively isolated, with no obvious nearby interacting companions in the immediate vicinity. The galaxy's overall morphology suggests a relatively quiescent state, with a low star formation rate.
