The galaxy appears to be an elliptical or lenticular galaxy, characterized by a smooth, relatively featureless morphology. It exhibits a high degree of central concentration, with a gradual decline in luminosity moving outwards from the core. No distinct spiral arms or bar structures are discernible in the image. The overall shape is close to circular with a small degree of ellipticity. There is no indication of recent or ongoing major merger activity, though there is some minor disturbance to the galaxy, possibly due to a small interaction with a smaller galaxy in the past. The colours indicate that it has a relatively old stellar population, with a lack of significant active star formation currently occurring. The galaxy's light is predominately redder in color due to the abundance of old stars.
