The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized light distribution. The shape is elongated, appearing cigar-shaped with the major axis significantly longer than the minor axis. The color profile suggests a population of older stars, trending towards redder hues in the central bulge and diminishing towards the outskirts. There is no visible evidence of spiral arms or active star formation regions within the galaxy. The galaxy exhibits a noticeable lack of dust lanes or other disruptive features, indicating a relatively quiescent state, and little to no indication of recent mergers or tidal interactions. Overall, the galaxy appears to be a well-formed, mature elliptical galaxy.
