The galaxy appears to be a lenticular or possibly an elliptical type, exhibiting a predominantly smooth, spheroidal morphology. It displays a cigar-like shape, with the major axis significantly longer than the minor axis. The color gradient suggests a slightly redder hue in the central region, potentially indicating an older stellar population and a relatively low rate of star formation throughout the galaxy. There's no clear evidence of spiral arms or significant disk structure. Faint disturbances or tidal features may be present, but they do not indicate recent major mergers, though a possible minor interaction cannot be ruled out. The overall light distribution is centrally concentrated, with a gradual decrease in surface brightness outwards.
