The galaxy presents as a relatively smooth, elliptical structure with a prominent central bulge. The core region exhibits a concentrated, luminous yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the galaxy exhibits a fainter, more diffuse reddish-orange color gradient along its major axis, possibly indicative of a decreasing concentration of older stars or a greater presence of dust obscuration. The overall morphology is elongated, with a cigar-like shape. There is no obvious evidence of spiral arm structure or ongoing major merging activity. Subtle irregularities within the outer halo may suggest minor gravitational interactions, but these are not prominent. The galaxy appears relatively isolated with no apparent tidal streams or other debris indicative of recent or ongoing disruptive events.
