The galaxy presents as an elliptical morphology, appearing generally smooth with a notable absence of distinct spiral arms or a prominent disk structure. It exhibits a moderately elongated shape, close to cigar-shaped. The central region displays a concentrated luminosity, suggesting a dense stellar population, while the outer regions gradually fade, implying a decreasing stellar density with increasing radius. The galaxy exhibits a color gradient, transitioning from a yellowish core to a slightly bluer hue towards the outer edges, indicative of subtle variations in stellar population age and composition across the galaxy. No obvious signs of tidal disturbances, major mergers, or significant star formation regions are readily apparent in this observation.
