The galaxy presents as a relatively smooth, elliptical or lenticular structure. It exhibits a concentrated central bulge that appears yellowish-orange, possibly indicative of an older stellar population. The overall shape is elongated, appearing cigar-shaped. There is a slight hint of a disk component. There is no obvious presence of spiral arms or strong features suggesting ongoing major mergers or significant tidal disturbances. The galaxy is slightly tilted relative to our line of sight. It presents as relatively isolated, without any obvious companions or signs of interaction with other galaxies in the immediate vicinity.
