The galaxy presents as an elliptical or lenticular system, appearing elongated with an approximate cigar shape. Its overall structure is smooth and concentrated, with a central bulge that shows a gradual decrease in luminosity outwards. The central region has a more yellow hue indicating an older stellar population and/or a higher dust content, whereas the outer regions exhibit bluer, more diffuse light. There is no apparent spiral arm structure or significant dust lanes visible in this image. No major interactions or mergers with other galaxies are readily apparent, only possible minor disturbances. The galaxy appears relatively isolated, suggesting it has evolved primarily through internal processes rather than strong gravitational interactions with neighboring systems.
