This galaxy appears to be a relatively smooth object with a slightly elongated, cigar-like morphology. The light distribution is centrally concentrated, with a bright nucleus that fades gradually outwards. The overall color of the galaxy is relatively blue in the inner regions transitioning to redder hues at the outer edges. This color gradient could potentially suggest ongoing or recently ceased star formation in the central regions, with an older stellar population dominating the outer halo. The morphology seems largely undisturbed; there are no clear signs of major mergers or significant tidal interactions. The galaxy seems to be relatively isolated with no obvious companion galaxies nearby. Overall, the galaxy appears to be a disk-like galaxy, possibly an early-type spiral or a lenticular galaxy, based on the smooth light distribution.
