The observed galaxy presents as an elliptical morphology, with a smooth, centrally concentrated luminosity profile. The core is bright and somewhat diffuse, indicating a high stellar density. The galaxy exhibits a noticeable flattening, with the major axis extending roughly three times the length of the minor axis. The color profile appears relatively uniform across the galaxy, trending towards a redder hue. There is no visible evidence of spiral arms, dust lanes, or recent star formation regions within the visible spectrum. Based on the overall structure, the galaxy is likely an elliptical galaxy.
