The galaxy presents a lenticular morphology, appearing as a somewhat flattened disk when viewed from our perspective. The central bulge is prominent, exhibiting a bright, yellowish hue, suggesting an older stellar population. Extending outwards from the bulge, a faint, elongated disk is visible. The disk structure appears relatively smooth, with only subtle variations in color and brightness, potentially indicating a lack of significant recent star formation. The overall shape is not perfectly circular, showing a slight elongation and some asymmetry, perhaps due to past interactions or internal dynamics. No obvious spiral arms are discernible. The galaxy is not undergoing any major merging events, and shows no signs of major disturbances.
