The galaxy presents as a slightly elongated, centrally concentrated object. It appears to have a smooth texture with no distinct spiral arms or bar structure visible. The core is a bright, yellowish-white, suggesting an older stellar population dominating the central region. Moving outward from the core, the galaxy fades into a more diffuse bluish haze, hinting at the presence of a younger, bluer stellar population in the outer regions, possibly indicating ongoing or recent star formation. The overall shape leans towards a flattened spheroid, although a cigar shape is not completely ruled out. There is no obvious evidence of major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed.
