The galaxy presents a generally elliptical morphology, with a noticeable central bulge that appears to be its brightest region. The overall color of the galaxy is consistent with an older stellar population, with a yellowish hue concentrated in the central region, suggesting a dominance of evolved stars. There is evidence of some internal structure within the galaxy, with slightly redder, less concentrated patches appearing around the main central bulge. These patches may indicate regions of on going star formation. The outer regions fade gradually, without a sharp edge, indicating a smooth transition in stellar density. The galaxy is relatively isolated in this field, and its shape does not seem to be significantly distorted, suggesting it hasn't undergone a major merger recently.
