The galaxy appears to be an elliptical type, characterized by its smooth, centrally concentrated light distribution. The core exhibits a bright, unresolved nucleus, suggesting the presence of a supermassive black hole or a region of intense star formation. Moving outwards from the core, the light gradually diminishes in intensity. A faint, reddish hue is slightly visible in the disk, possibly indicating a population of older stars or dust lanes. While the galaxy's overall shape is generally smooth, there are subtle indications of minor disturbances or tidal features, such as faint asymmetries, suggesting possible past or ongoing interactions with smaller companion galaxies. There does not appear to be a pronounced spiral structure, nor is there evidence of a significant amount of blue light indicative of active star formation.
