The galaxy presents an elongated, elliptical morphology. The central bulge exhibits a concentrated, yellowish hue, suggesting an older stellar population. Moving outward from the core, a subtle gradient to slightly bluer tones is observed, possibly indicating regions with ongoing, albeit low, star formation. There is a hint of a faint, extended disk component, but the image quality limits detailed assessment. The galaxy does not display any obvious signs of a major merger or significant tidal disturbances. The smooth light distribution is interrupted by only subtle features. Overall, the galaxy appears as a relatively quiescent system.
