The galaxy presents a generally smooth appearance, with a concentration of light towards the center. There's a slight ellipticity, suggesting it is not perfectly round. Faint, diffuse features are visible extending outwards from the central region, potentially indicative of a disk structure or tidal disturbances. The color profile shifts from a yellowish-white core to bluer hues in the outer regions. This may be an indicator of differing stellar populations, with older, redder stars dominating the core and younger, bluer stars present in more extended arms or regions of star formation. There is some indication of a possible ongoing or past merger event due to the disturbances in the galaxy's morphology, but it could be a relatively minor disturbance.
