The observed galaxy exhibits a moderately elliptical morphology. A central bulge region displays a bright, cyan-colored luminosity, suggesting ongoing star formation. The galaxy is moderately sized and exhibits a noticeable disk-like structure, and is not perfectly uniform. Faint, extended arms or tidal features are not clearly visible, indicating a relatively undisturbed system. The color profile suggests a mixture of stellar populations within the galaxy. The core region shows evidence of younger, hotter stars, while the outer regions indicate the presence of older, redder stars. The galaxy displays minor distortions, with a slight elongation. Some minor disturbances are present, but the system doesn't seem to show any major interactions. A small reddish region is visible on the outer perimeter of the galaxy. Overall, the galaxy appears as an isolated object, without any major signs of an ongoing merger or interaction.
