The galaxy appears as a moderately bright, relatively compact object. It exhibits a largely smooth, elliptical morphology with a high degree of central concentration. There is a noticeable absence of distinct spiral arms or a well-defined disk structure. The galaxy's color profile suggests a mix of stellar populations, with a slightly redder core and bluer outer regions. This is indicative of older stars concentrated in the central bulge and younger stars populating the outskirts. There are no obvious signs of a recent major merger event or strong tidal disturbances, though some subtle irregularities in the outer isophotes might suggest minor past interactions. The overall appearance aligns with that of an early-type galaxy, potentially an elliptical or lenticular galaxy undergoing relatively low levels of star formation.
