The galaxy presents as an elliptical morphology, elongated in shape with a cigar-like appearance. It displays a smooth and largely featureless light distribution, suggesting a lack of prominent spiral arms or dust lanes. The central region exhibits a higher surface brightness, indicative of a concentrated core. Color gradients are subtle, with a general trend towards bluer hues at the outer edges of the galaxy and yellower hues towards its center, perhaps suggesting older stellar populations concentrated towards the core. There is no immediately obvious evidence of ongoing major merger activity, although the outer regions show a slight irregularity, potentially pointing to past minor interactions or accretion events. Overall, the galaxy appears to be a relatively evolved system with a quiescent star formation rate.
