The galaxy presents as a lenticular or possibly an elliptical type system, characterized by a smooth, elongated morphology. The central bulge appears prominent and exhibits a yellowish-white color, likely indicating an older stellar population. Moving outward, the galaxy exhibits a faint, diffuse disk structure with a subtle bluish hue, suggesting the presence of some younger stars and ongoing star formation, though at a modest rate. The galaxy's overall light distribution is relatively uniform, lacking strong spiral arms or prominent dust lanes. A noticeable elongation is present, possibly indicative of a cigar-like shape. The system does not show any obvious signs of major mergers or tidal disturbances, suggesting it is a relatively undisturbed galaxy. There may be a very slight asymmetry or minor irregularity in the outer regions of the galaxy.
