The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The core region exhibits a yellowish-orange hue, suggestive of an older stellar population dominating the light output. Moving outwards from the center, the color transitions to a more subtle blue-green tint, potentially indicating the presence of some younger, hotter stars or ionized gas, although this is less pronounced. The galaxy appears largely elliptical in shape, with no clear spiral arm structure or significant morphological disturbances visible. There is a slight elongation evident, suggesting it is not perfectly spherical. The overall smooth appearance and color distribution suggest a relatively evolved system, possibly an early-type spiral or lenticular galaxy. However, the slight color variations hint at a low level of ongoing star formation activity.
