This galaxy exhibits a generally elliptical morphology, appearing elongated rather than perfectly circular. The central region presents a noticeable concentration of light, suggesting a prominent galactic nucleus or bulge. Color gradients are subtle, with the core displaying a yellowish-orange hue, possibly indicative of an older stellar population. Fainter, bluer regions are observed extending from the central area, hinting at the presence of younger stars or ongoing star formation, but the overall star formation rate appears to be relatively low. A slight asymmetry is visible in the distribution of light, which may suggest a minor tidal disturbance or interaction with a smaller object. There is no definitive evidence of well-defined spiral arms or a prominent disk component; its overall structure is more consistent with that of an early-type galaxy.
