The galaxy presents an elongated, cigar-shaped morphology. Its light profile suggests a relatively smooth distribution, with a bright, concentrated core that gradually fades towards the outer edges. The central region exhibits a yellowish hue, potentially indicating a population of older stars. The outer regions appear slightly bluer, which may be indicative of some star formation activity, although at a low rate. There is no visual evidence of spiral arms or a prominent disk structure. The overall appearance is consistent with that of an elliptical galaxy, though it cannot be ruled out that this is a highly inclined spiral. There do not appear to be any signs of ongoing mergers or major tidal disturbances.
