The galaxy appears to be a relatively compact object, exhibiting a smooth, elliptical morphology. Its light is concentrated towards the center, suggesting a prominent galactic nucleus or bulge. There is a gradient of light intensity diminishing outwards from the central region, with no apparent spiral arm structures or distinct features indicative of active star formation. The galaxy appears largely homogeneous in color across its surface, with a slightly reddish hue, suggesting an older stellar population and a lack of ongoing significant star formation. The shape of the galaxy is nearly circular. There is no visual evidence of tidal tails, ongoing mergers, or significant disturbances in its structure.
