The galaxy presents as a primarily smooth, elliptical structure, exhibiting a notable lack of defined spiral arms or a prominent disk. Its shape deviates from a perfect circle, showing an elongated, cigar-like morphology. The central region displays a concentration of light, suggesting a dense nucleus. The galaxy exhibits a color gradient, transitioning from a redder hue in the core to a slightly bluer, albeit still relatively smooth, outer region. There are some faint indications of possible minor disturbances in the outer halo, but no clear evidence of ongoing major mergers or tidal interactions. The overall appearance suggests a galaxy dominated by an older stellar population, with a relatively low star formation rate.
