The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light profile with a somewhat elongated shape. The central bulge is the brightest region, characterized by a yellow hue, likely indicating an older stellar population. There is a slight flattening visible, suggesting it is not perfectly spherical. No distinct spiral arms or dust lanes are discernible. The galaxy appears to be relatively isolated with no indications of a major merger. There is what appears to be a small object in the upper left, but it is uncertain if it is associated with the galaxy, though they appear to be a similar hue. There are no signs of strong tidal features or significant star formation activity. The overall morphology suggests a galaxy that has largely exhausted its gas reservoir and is dominated by evolved stars.