The galaxy presents as a largely featureless, elliptical morphology. Its light profile is dominated by a smooth, centrally concentrated component, suggesting an older stellar population. The core exhibits a yellowish hue, possibly indicative of evolved stars. There is a gradual decrease in brightness towards the outer regions, with no distinct spiral arms or prominent dust lanes visible. The galaxy appears relatively isolated, showing no significant tidal distortions or signs of recent merger activity. It has a generally rounded appearance, showing no elongation. The galaxy is in a relatively early stage, showing a generally smooth profile. 
