The galaxy presents a somewhat elliptical morphology, appearing elongated in shape. Its color profile indicates a predominantly older stellar population, with a yellowish hue concentrated towards the central region. Fainter blue components exist toward the edges, suggesting younger stars are present, though less abundant. The galaxy appears relatively smooth in texture, with no distinct spiral arms or prominent dust lanes visible at this resolution. A very slight asymmetry is observed in the shape, possibly suggesting a minor gravitational interaction or recent accretion event, though no tidal tails or major disturbances are apparent. The overall structure seems well-defined, indicating a gravitationally bound system.
