The galaxy presents as an elongated, cigar-shaped structure. The core region exhibits a bright, somewhat diffuse glow, potentially indicating a high concentration of stars or active galactic nucleus activity. The overall color gradient shifts from a bluer hue at one end to a slightly redder tone at the other, possibly reflecting variations in stellar populations and dust distribution across the galactic body. There appears to be a general smoothness to the galaxy’s light distribution, though subtle irregularities may suggest minor internal disturbances or interactions. No distinct spiral arm structure is clearly discernible, indicating that this galaxy may be either an elliptical or lenticular type. The galaxy is relatively isolated, with no immediately apparent signs of ongoing major mergers or tidal interactions.
