The galaxy presents as a disk-shaped object, viewed nearly edge-on. It exhibits a prominent central bulge or core region, appearing brighter and more condensed than the surrounding disk. The disk structure is relatively smooth and appears to lack defined spiral arms. There's a slight asymmetry in the disk's light distribution, suggesting potential gravitational interactions or recent accretion events. The color gradient observed reveals bluer hues towards the outer edges of the disk, suggesting the presence of younger, hotter stars, and redder hues are more concentrated towards the central bulge, indicative of an older stellar population. Overall, the galaxy displays a mixture of features characteristic of both spiral and lenticular galaxies, showing features of smoothness more than disk structures. There are faint hints of disturbances potentially indicative of minor mergers or tidal interactions.
