The galaxy appears to be an elliptical galaxy, characterized by a generally smooth and round morphology. There is a noticeable concentration of light towards the center, suggesting a prominent galactic nucleus. The color profile is generally redder, hinting at an older stellar population with a reduced rate of star formation. While mostly homogenous, there are slight variations in the light distribution that might imply minor disturbances or interactions in its past. No spiral arms or significant dust lanes are obviously visible at this resolution.
