The galaxy presents as a centrally concentrated object, exhibiting a smooth and largely featureless morphology. The light distribution appears roughly circular with a distinct core. There is a faint but discernible extended halo surrounding the central concentration. The color profile suggests a relatively old stellar population throughout the structure, given the subtle reddish hue, implying an older generation of stars. There is no obvious spiral structure or significant dust lanes visible. There appears to be a slight disturbance towards the upper right corner of the galaxy. The galaxy appears to be relatively isolated, with no other obvious major galaxies in close proximity that would suggest a recent or ongoing major merger event.
