The galaxy presents as a relatively smooth, elliptical structure. It has a concentrated central bulge with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a yellowish-red hue, indicative of an older stellar population with minimal ongoing star formation. There is a general lack of distinct spiral arm features or prominent dust lanes suggesting a more evolved system. The overall morphology suggests a spheroid-dominated galaxy, likely a massive elliptical with a high stellar mass. No significant tidal features or signs of recent merger activity are readily apparent. The galaxy appears to be relatively undisturbed and relaxed in its morphology.
