The galaxy presents as a luminous, elongated structure, likely a disk galaxy viewed at an oblique angle. The central region exhibits a concentrated brightness, suggesting a prominent galactic bulge. This bulge appears relatively smooth and featureless at this resolution, indicative of an older stellar population. The disk component displays a subtle color gradient, transitioning from a bluer hue at the outer edges to a yellower tone closer to the core. This could imply ongoing or recent star formation in the outer regions, contrasted with an older stellar population dominating the inner parts. Faint and diffuse extensions emanate from the main body of the galaxy. These features might be indicative of tidal tails or disrupted structures resulting from a minor gravitational interaction, although no clear signs of a major merger are apparent. The galaxy appears relatively isolated in its immediate vicinity.
