The galaxy presents a generally smooth morphology, appearing as an elliptical or lenticular type. Its shape is elongated, exhibiting a cigar-like appearance. The central bulge is prominent and displays a bright, yellowish-white color, suggestive of an older stellar population. Moving outward from the core, the color transitions toward a slightly bluer hue, especially at the outer edges, which may indicate the presence of some younger stars or ongoing star formation, though at a relatively low rate. There are no clear signs of spiral arms or a well-defined disk structure. No major mergers or tidal disturbances are evident, although there might be subtle irregularities in the outer regions. Overall, the galaxy seems relatively undisturbed.
