The galaxy presents a primarily smooth morphology, suggesting it is likely an elliptical or lenticular type. Its overall shape is somewhat elongated, appearing to be slightly more 'in between' round and cigar-shaped. There is a central concentration of light that is bright and yellowish-white in color. This likely signifies an older stellar population. The outer regions of the galaxy exhibit a gradual fading in luminosity, with a reddish hue to its outer edges. No significant signs of spiral arms or active star formation are readily apparent in this image. There are possible hints of minor disturbance, but no apparent features indicating a major ongoing merger event. Overall, this appears to be a relatively undisturbed galaxy with evidence of an older stellar population and minimal ongoing star formation.
