The galaxy presents as a generally smooth structure, exhibiting a slightly elongated, cigar-like shape. There is a bright central bulge which seems to dominate the overall light emission. The galaxy's color profile appears to shift from a yellow-white core to a redder hue toward its outer edges. There is no clear visual indication of spiral arm structures or dust lanes, suggesting a morphology leaning towards an elliptical or lenticular type. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of ongoing major mergers or tidal disruptions. The rate of new star formation is probably quite low.
