The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. It exhibits a slightly elongated morphology, deviating somewhat from a perfect circular shape. The central region displays a brighter, more condensed concentration of light, suggestive of a possible galactic nucleus or a dense stellar population. A faint extension or tidal tail appears to emerge from one end, potentially indicating past or ongoing gravitational interactions. Color gradients within the galaxy are subtle, with the central region showing a slightly yellower hue compared to the outer regions, which appear bluer. This could indicate differences in stellar populations, with older, redder stars dominating the central bulge and younger, bluer stars residing in the outer regions or extensions. There appears to be a very slight disturbance in the light distribution of the galaxy. Overall, this galaxy appears to be in the process of some sort of interaction.
