The galaxy presents as a somewhat elongated, disk-like structure viewed at an oblique angle, suggesting a possible spiral or lenticular morphology. The central region exhibits a concentrated, yellowish-white hue, indicative of an older stellar population. There is a subtle color gradient extending outwards from the center, with the outer regions displaying a slightly bluer tinge, potentially suggesting the presence of younger, hotter stars or ongoing star formation. The overall structure appears relatively smooth, with no prominent spiral arms immediately apparent in this image. There is a very faint hint of asymmetry or distortion in the outer disk, warranting further investigation into possible past or ongoing interactions. The galaxy is relatively compact and appears to be of moderate size.
