The galaxy presents as a relatively smooth, elliptical morphology, elongated along its major axis. The central bulge exhibits a brighter, yellowish hue, indicating a population of older stars. A subtle blueish halo surrounds the central region, suggesting the presence of some younger stars and ongoing, albeit low, star formation. The absence of distinct spiral arms or a prominent disk further reinforces its classification as an elliptical galaxy. There is no discernible evidence of a major merger or significant tidal disturbances, although the slight asymmetry could indicate a past minor interaction. Overall, the galaxy appears to be a relatively quiescent system, with a moderately high mass and correspondingly low specific star formation rate.
