The galaxy presents a largely smooth, elliptical morphology. It appears generally rounded in shape, with a high degree of central concentration. There is little evidence of spiral arms or a well-defined disk structure. The galaxy's color is predominantly yellowish-orange, with the core appearing more intensely yellow. This suggests a stellar population dominated by older, redder stars and potentially a lower rate of ongoing star formation. While the primary structure is smooth, there are indications of minor irregularities, particularly near the outer edges of the galaxy's luminous profile. The light distribution tapers off gradually from the central bulge outward. There are no visible signs of a major ongoing merger.
