The galaxy appears as an elongated, disk-like structure exhibiting a smooth morphology. The central bulge displays a yellowish hue, suggesting an older stellar population. Moving outwards from the bulge towards the galactic disk, the color transitions to a slightly bluer tone, indicative of more recent star formation regions. There are no readily apparent spiral arm structures, or a large central bar; the disk appears largely amorphous and relatively featureless in terms of distinct morphological components. The overall shape is moderately inclined with respect to our line of sight, allowing us to observe the galaxy as a flattened ellipse. The galaxy does not appear to be undergoing any major mergers or significant tidal interactions with nearby galaxies.
