The galaxy presents an elongated, roughly elliptical morphology. There is a high degree of central concentration, indicating a prominent bulge. The light distribution appears relatively smooth, suggesting a lack of significant spiral arm structure. A faint, extended halo is barely discernible surrounding the central region. The galaxy appears to be inclined with respect to the line of sight, as evidenced by its flattened shape. The colors are relatively uniform across the galaxy, hinting towards a lack of significant recent star formation. There are subtle hints of structural irregularities or minor disturbances on the outskirts, possibly indicative of past interactions or mergers.
