This galaxy presents a relatively smooth, elliptical-like morphology. The central region exhibits a high concentration of light, appearing nearly spherical. The color profile suggests an older stellar population dominating the galaxy, indicated by the yellowish-white hue concentrated towards the center. There's some evidence of bluer tones in the outer regions, potentially indicating ongoing, albeit relatively low, star formation. Overall, it appears to be a fairly isolated system, with no obvious signs of a major merger or significant tidal disturbances. It is unlikely to be a late-type spiral galaxy and lacks distinct spiral arm structures. The galaxy displays a moderate inclination relative to our line of sight.
