The galaxy appears to be an elliptical galaxy, exhibiting a smooth and relatively featureless morphology. It presents a near-spheroidal shape with a slight elongation. The light is concentrated towards the center, with a gradual decrease in surface brightness towards the outer regions. The color profile suggests a predominantly older stellar population, with a yellowish-orange hue indicating a lack of significant ongoing star formation. No spiral arms, dust lanes, or prominent star-forming regions are discernible within the available resolution. There is no apparent evidence of recent or ongoing major mergers or significant tidal disturbances affecting the galaxy's overall structure. Subtle indications of minor disturbances can neither be confirmed nor completely ruled out due to the image's limitations.
