The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. There is an absence of readily apparent spiral arms or prominent dust lanes. The primary color of the galaxy appears to be a yellowish-orange hue, suggestive of an older stellar population dominating the light output. The galaxy appears to be somewhat elongated, deviating slightly from a perfectly circular profile. Faint, diffuse light extends outwards from the central core, gradually fading into the background sky. There may be some slight tidal distortions of the galaxy, but further analysis would be needed to confirm.
