The galaxy presents an elongated, elliptical morphology. It exhibits a smooth, diffuse structure with a concentration of light towards the central region, suggesting a bulge. The color profile indicates a dominant population of older stars, particularly within the bulge, characterized by a redder hue. A subtle disk-like feature is visible, extending from the bulge. There appears to be ongoing, but low star formation within the galaxy, as indicated by the presence of bluer regions sparsely scattered throughout. The overall form lacks significant signs of tidal disruption or major mergers, though minor disturbances cannot be ruled out due to the resolution. The galaxy's shape can be described as an oval or ellipse, with a ratio between major and minor axes suggesting a moderate inclination. The appearance is consistent with an early-type spiral galaxy viewed at an angle.
