The galaxy presents a primarily smooth morphology, indicating characteristics of an elliptical or lenticular type. The central bulge exhibits a high degree of concentration, appearing nearly spherical. The color profile of the galaxy transitions from a yellowish-white core to a reddish hue in the outer regions. This coloration is consistent with an older stellar population, where the more massive, shorter-lived stars have evolved off the main sequence. There's very little to no indication of spiral arm structure or significant dust lanes. A subtle distortion in the outer regions is potentially indicative of a minor interaction or past merger event, although the dominant impression is one of overall regularity.
