The galaxy presents a primarily smooth, elliptical morphology. It exhibits a concentrated central bulge, indicating a high stellar density. The color profile suggests a relatively older stellar population with a slight bluer hue in the outer regions. There is only a vague hint of any spiral structure and the disk, if present, is very subdued. Overall, the galaxy appears relatively isolated, showing no strong evidence of recent or ongoing major merger activity. There is some slight indication of a minor disturbance in the galaxy's form.
