The galaxy presents as an elongated, disk-shaped structure with a bright, concentrated central bulge. The primary axis of the galaxy is oriented at roughly 45 degrees relative to the horizontal. The luminosity is centrally concentrated, decreasing gradually towards the outer edges. The apparent flattening suggests it is observed at a high inclination angle, as the ratio between its semi-minor and semi-major axes is about 0.4. There is a hint of spiral arm structure faintly visible, but they are not well-defined. The colour appears yellow-white, hinting at a mix of stellar populations, with a possibly older stellar population dominating the bulge region. A faint, blue feature is visible in the central region, possibly indicating a region of more active star formation. There is no evidence of strong tidal features or signs of recent major mergers within the galaxy's immediate environment based on the image.
