The galaxy presents as a centrally concentrated object with a generally smooth morphology. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. This core smoothly transitions into a fainter, diffuse outer halo. There is a very slight indication of possible spiral structure. A minor degree of disturbance is present, which could indicate ongoing interactions. The galaxy appears relatively round in shape. The color gradient shifts towards redder tones from the center outwards, which is consistent with a decline in star formation activity away from the core.
