The galaxy appears as a faint, elongated structure with a smooth overall appearance. Its shape is decidedly cigar-shaped, with a length-to-width ratio indicating a flattened, but not completely disklike structure. There is no obvious central bulge or distinct spiral arm structure visible. The color profile suggests a population of older stars, as the galaxy exhibits a relatively redder hue. There are no noticeable signs of active star formation, such as bright blue regions or HII regions. The overall appearance is undisturbed, with no obvious signs of a recent merger or tidal interactions, although a minor disturbance cannot be ruled out. The galaxy presents as a relatively isolated system, without close companions.
