The galaxy presents as a single, relatively smooth object with a generally elliptical morphology. It displays a concentrated central region exhibiting a high degree of sphericity. The color profile suggests a mature stellar population, with a yellowish-red hue indicating a dominance of older, redder stars and relatively low ongoing star formation. There is no apparent spiral structure, bar, or other disk-like features visible. Faint deviations and irregular details, possibly indicative of very minor disturbances, are present in the outer regions, but the galaxy's overall structure is largely undisturbed. The galaxy shows little evidence of significant ongoing merging activity.
