The galaxy presents as a largely homogenous elliptical system. It appears smooth with a highly concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. There is a slight extension of the galaxy along its major axis, hinting at a weakly cigar-like shape, though it primarily presents as round. There is no visible evidence of spiral arms, a prominent disk, or strong tidal disturbances suggestive of recent major merger activity. A faint red halo is visible at the periphery of the galaxy, indicating a degree of ongoing, albeit low, star formation within the system. The overall color profile indicates the presence of evolved stars and a relatively quiescent star formation history.
