This galaxy exhibits a somewhat amorphous morphology, lacking a well-defined spiral or elliptical structure. There is an overall smoothness to its light distribution, with a central, brighter region surrounded by a more diffuse halo. The light appears to be yellowish-white in the central region, indicative of an older stellar population, while the outer regions show a slightly bluer hue, potentially signifying the presence of younger, hotter stars and ongoing star formation activity. A faint asymmetric extension is apparent on one side of the galaxy, which may be a tidal feature resulting from a past interaction, hinting at a possible ongoing or recent merger event. Overall, the galaxy appears to be undergoing a process of morphological disturbance and star formation.
