The galaxy presents an overall smooth appearance, with no distinct spiral arm structures or prominent dust lanes readily apparent. The central region exhibits a concentrated, bright core, potentially indicative of an older stellar population. The color gradient transitions from a yellowish-white core to a bluer hue in the outer regions. The galaxy appears elongated, deviating significantly from a perfectly circular morphology, indicating a possible ellipsoidal shape or a disk-like structure viewed at an angle. There are no signs of strong tidal features or ongoing major mergers. Subtle irregular structures or minor disturbances may be present within the galaxy's outer regions, but further investigation would be needed.
