The galaxy appears to be a relatively smooth elliptical or lenticular type, exhibiting a concentrated central bulge that transitions gradually into a less dense halo. There is a slight suggestion of a disk component, but it is not clearly defined. The galaxy displays an overall rounded morphology, deviating little from a circular form.

The color profile indicates an older stellar population, with a dominant yellowish-orange hue in the central bulge and a subtle bluer tint in the outer regions. The light distribution suggests a more quiescent galaxy, lacking the distinct spiral arms or prominent star-forming regions usually associated with higher star formation rates. There are some signs of minor gravitational disturbances, or interactions with other galaxies. These disturbances are subtle.

The estimated size suggests a substantial galaxy. Considering these characteristics, it can be surmised that this galaxy is a massive object with a significant stellar mass and low specific star formation rate.
