The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. There is a distinct bulge component characterized by a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy show a more diffuse, bluish-white color, suggesting the presence of some younger stars or lower metallicity stars. The galaxy's overall shape is elongated, with an approximate axis ratio of 2:1, suggestive of an E4-E5 elliptical classification. There is no clear evidence of spiral arms, dust lanes, or significant tidal features. The galaxy does not appear to be undergoing any major mergers, though there may be evidence of a very minor disturbance or interaction, but this is difficult to ascertain given the image resolution. The object has an estimated size of around 4 kpc. 
