The galaxy presents as a moderately luminous, elongated object with a smooth, featureless morphology. The central region exhibits a concentrated, bright yellowish-white hue, suggesting a relatively old stellar population. Surrounding this core, a fainter, more diffuse, and slightly bluer halo extends, which is indicative of some ongoing star formation. The overall shape is somewhat cigar-like, displaying a noticeable deviation from a perfectly circular profile. No prominent spiral arms or irregular structures are discernible within the available image resolution, and there is no obvious signs of any major galactic merger or strong tidal disturbance, although there may be some minor disturbance evident. The observed color gradient, from the yellowish center to the bluish outer regions, implies a radial variation in stellar population and star formation activity.