The galaxy appears as a centrally concentrated object, exhibiting a generally elliptical morphology. The light distribution is fairly smooth, with a dominant central bulge region. The color profile suggests a population of older stars, with a relatively redder hue dominating the galactic body. There is a noticeable absence of distinct spiral arm structures or prominent dust lanes, implying it's likely an early-type galaxy. The galaxy is fairly compact, with a concentrated appearance indicative of a high stellar density. There's no obvious evidence of a recent major merger or tidal disruption. The image suggests the galaxy is in a relatively quiescent state.
