The galaxy presents as a disk galaxy, viewed at a high inclination relative to our line of sight. The primary body of the galaxy exhibits a relatively smooth, diffused light distribution, with a slightly brighter core region. There's a noticeable asymmetry in the outer halo, suggesting the presence of potential tidal disturbances. The central region shows a slightly bluer hue, which is consistent with some ongoing star formation activity. The overall color gradient transitions towards redder tones in the outer regions, possibly indicating an older stellar population. There's also evidence of possible faint tidal tails or streams, indicative of previous or ongoing interactions with other galaxies or intergalactic material. The disk appears relatively undisturbed, suggesting that the merger event, if present, may have been a minor one or is in its early stages.
