The galaxy presents a generally smooth appearance, with a somewhat elongated, cigar-like shape. The central region exhibits a bright, concentrated luminosity, likely indicative of a substantial stellar population within the galactic nucleus. The color gradient transitions from a yellow/white core to a cooler, bluer halo. A subtle disc-like structure may be present, but is not well defined. There appear to be minor disturbances in the galaxy's structure, perhaps signs of a minor interaction or internal dynamics. The lack of prominent spiral arms and relatively smooth light distribution suggest the galaxy is an elliptical or lenticular type. Overall, this galaxy appears to be relatively massive with a low star-formation rate.
