The galaxy presents as an elliptical morphology, with a high degree of central concentration. The color profile indicates an older stellar population dominating the core, characterized by a yellowish-orange hue. There appears to be a faint, somewhat diffuse disk component exhibiting bluer tones, extending asymmetrically from the central bulge. This feature suggests the presence of ongoing, albeit limited, star formation activity. While a majority of the galaxy shows a smooth appearance, there is a hint of a minor tidal disturbance on one side, potentially indicating a past or ongoing interaction. The overall structure is slightly elongated, departing from a perfectly circular form. There is no clear evidence of a major merger event or strong spiral arm structure, suggesting a galaxy that has largely settled into a more quiescent state.
