The galaxy presents as an elongated, relatively smooth structure, indicative of an elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars or an active galactic nucleus. The light distribution decreases gradually from the core outwards. The galaxy does not display prominent spiral arms or distinct dust lanes. There is a slight bluing of the light at the edges. Overall, the galaxy appears well-defined with no significant signs of ongoing major merger activity.