The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology with minimal discernible features. The light profile suggests a concentrated central bulge region that transitions gradually into an extended, fainter halo. The galaxy presents a yellowish hue, potentially indicative of an older stellar population dominating the overall light emission. There is no evidence of spiral arms or a prominent disk structure. No signs of active galactic nuclei activity or ongoing major mergers are readily apparent. There are no features suggesting recent or ongoing star formation.