The galaxy presents a largely smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge, brightest in the green-yellow portion of the spectrum, surrounded by a more diffuse halo. The galaxy has a generally rounded shape, with no obvious tidal features or distortions indicative of a recent major merger. Faint blue-tinged areas suggest a low level of ongoing star formation, while the dominant yellow and red hues are more likely to be representative of an older stellar population. Overall, the galaxy appears to be relatively isolated and undisturbed, with only minor asymmetry visible.
