The galaxy presents as a moderately luminous, relatively compact structure exhibiting a predominantly elliptical morphology. The central region displays a high degree of surface brightness, appearing smooth and concentrated. Proceeding outwards from the core, the luminosity gradually diminishes, indicating a decreasing stellar density. There appears to be a slight asymmetry to the galaxy, with a faint extension emanating from the core. The color profile shows a transition from a warmer, yellowish hue at the core, possibly indicating an older stellar population, to slightly cooler, bluer tones in the outer regions, which could imply the presence of some younger stars or regions of ongoing star formation, though limited. Overall, the galaxy appears relatively undisturbed, without prominent tidal features, but may be in a state of interaction with a smaller galaxy.
