The galaxy presents a generally smooth and rounded morphology. The light distribution appears centrally concentrated with a slight decrease in intensity outward from the core. There is a lack of any obvious spiral arm structure or prominent disk features. The galaxy exhibits a pale blue hue, suggestive of a moderate amount of recent or ongoing star formation, but the overall color implies a potentially aging stellar population. There is no clear evidence of significant tidal disruption, major mergers, or strong gravitational interactions in this image.