The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light profile appears diffuse with a gradual decline in intensity from the core outwards, lacking distinct spiral arm features. Coloration suggests an older stellar population, evidenced by the yellow-orange hue dominant throughout the galaxy, possibly indicative of lower levels of on-going star formation. The apparent round morphology suggests it is viewed close to face-on, with little indication of significant dust lanes or irregular shapes indicative of recent major mergers. There are some slight irregularities to the structure that could mean minor disturbances are happening.