The galaxy presents as a relatively smooth, elliptical structure, with a high degree of central concentration. The core exhibits a yellowish-white hue, indicative of an older stellar population, likely dominated by evolved, lower-mass stars. Moving outward from the core, the color transitions to a slightly bluer shade, suggesting the presence of some younger, hotter stars, though not in substantial quantities. There are no distinct spiral arms or prominent dust lanes visible, supporting the classification as elliptical. The isophotes appear generally regular and undisturbed. No signs of ongoing major mergers are apparent. The overall morphology implies a quiescent galaxy, with a low star formation rate. The galaxy displays an elongated shape, though it appears closer to round than cigar-shaped.
