The galaxy presents as a somewhat elongated, elliptical morphology. It exhibits a generally smooth, featureless appearance, suggesting an absence of prominent spiral arms or strong dust lanes. The color gradient is subtle, with a slightly bluer central region transitioning to redder hues in the outer regions. This could indicate a higher concentration of younger, hotter stars in the core compared to an older stellar population dominating the periphery. There is no strong evidence of tidal disturbances or merging activity, suggesting a relatively isolated system that has evolved largely undisturbed. The overall structure appears regular and well-defined, consistent with an early-type galaxy classification.
