The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. The galaxy exhibits a distinct yellowish-orange hue, indicative of an older stellar population. There is no apparent disk structure, spiral arms, or significant dust lanes visible. Its shape is mostly round, with minimal elongation. No signs of tidal disturbances, major mergers, or strong interactions with other galaxies can be seen. The light profile appears to decline gradually from the center outward, with no obvious knots or bright star-forming regions.
