The galaxy appears to be a relatively smooth, single structure. Its overall morphology suggests a possible elliptical galaxy, exhibiting a generally rounded shape with a slight elongation. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy displays a noticeable color gradient; the central region exhibits a yellowish-orange hue, transitioning to redder tones in the outer regions. This color profile may indicate an older stellar population dominating the central regions, with comparatively younger, possibly star-forming regions located further out. There appears to be no distinct spiral arm structure or significant dust lane features visible. There are suggestions of minor disturbances within the galaxy, however no major merging events or tidal tails appear to be present.
