The galaxy appears as a centrally concentrated, luminous object with a smooth, spheroidal morphology. There is little evidence of spiral arms or a prominent disk structure. The galaxy exhibits a yellowish-white hue, indicative of an older stellar population and a relatively low rate of ongoing star formation. The shape is moderately elliptical. There are no obvious signs of recent major merger activity, but the image does suggest subtle disturbances in the outer regions of the galaxy, possibly indicating a minor interaction or past accretion event. The galaxy exhibits a moderate redshift, suggesting it is a relatively distant object.
