The galaxy appears as a relatively smooth, centrally concentrated object with a generally elliptical morphology. There are no prominent spiral arms or a distinct bar structure visible. The light distribution suggests a centrally dominant bulge component, and the overall shape seems relatively undisturbed, with little evidence of ongoing major merging activity, although there is the possibility of minor disturbances in the overall structure. The galaxy exhibits a colour gradient, appearing bluer in its central regions and becoming redder towards the outskirts, likely indicating a radial variation in stellar populations, with younger, bluer stars concentrated in the center and older, redder stars dominating the outer regions. The lack of significant dust lanes is also notable, which could indicate a relatively low gas content.
