The galaxy appears as an elliptical or lenticular type, exhibiting a relatively smooth light distribution with minimal discernible features. The central bulge is prominent and displays a yellowish-orange hue, suggestive of an older stellar population. The galaxy has a fairly symmetric morphology with a slight elongation. No spiral arms or significant dust lanes are apparent. The overall structure indicates that this galaxy is likely a well-established system, without any significant signs of recent major mergers or tidal disturbances. The color gradient suggests a passive evolution phase with a declining star formation rate.