The galaxy appears as a centrally concentrated, relatively smooth object. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outward from the center, the color transitions to a slightly bluer shade, possibly indicating the presence of some younger stars, though these are not distinctly resolved. The galaxy's overall shape is somewhat elliptical, with no obvious spiral arms or a bar structure. There is little evidence of significant dust lanes or prominent star-forming regions, but some minor disturbances may be present. The galaxy does not appear to be undergoing a major merger, though minor interactions cannot be ruled out based on the observed morphology.
