This galaxy presents as a relatively smooth, disk-dominated system. The central bulge exhibits a concentrated, yellowish-orange hue, suggesting an older stellar population with minimal ongoing star formation within the nuclear region. Extending outward from the bulge, a flattened disk is visible, although the image resolution limits detailed analysis of spiral arm structures. The disk appears less luminous and subtly bluer than the central bulge, potentially indicating the presence of younger, hotter stars. The galaxy is likely a high mass system with suppressed star formation. There is no evidence of strong tidal features or significant morphological disturbances, suggesting that it is not currently undergoing a major merger. It appears to be relatively undisturbed.
