The galaxy presents as a relatively smooth, elongated structure with a central bulge. It appears to be an elliptical galaxy with a noticeable halo of diffuse light surrounding the core. The light distribution suggests a lack of distinct spiral arms or intricate dust lanes. Color gradients are subtle, with a generally bluer hue in the central region, potentially indicating some active star formation, contrasted with the more reddish color towards its outer regions. The overall morphology is suggestive of an older stellar population with a relatively low star formation rate, with a possible minor interaction occurring with a near companion.
