The galaxy presents as a relatively smooth, elongated structure viewed at a significant angle to its plane, suggesting a disk-like morphology. The central region exhibits a concentrated, yellowish-white hue, potentially indicative of an older stellar population. Progressing outwards from the center, a subtle blue gradient emerges, suggesting the presence of younger, hotter stars within the galactic disk. The overall shape is suggestive of a flattened spheroid, and there appears to be little indication of ongoing major merging events or significant tidal disturbances. The light distribution is fairly even, with no pronounced spiral arms or bar structures immediately apparent in this resolution. The object does appear to be a highly tilted disk galaxy, based on its shape.