The galaxy presents an elongated, cigar-shaped morphology, indicative of a potentially elliptical or lenticular system viewed at an oblique angle. A notable central bulge is observed, characterized by concentrated light, suggesting a higher stellar density compared to the outer regions.

The color distribution across the galaxy shows a subtle gradient. The core exhibits a yellowish-white hue, potentially indicating an older stellar population and a paucity of active star formation. Moving outward from the core, the colors tend toward blue, suggesting the possibility of younger stars or the presence of some star formation within the disk or spiral arms that may not be clearly discernible in this image.

There appears to be no evidence of significant tidal disruption or ongoing merger activity; the galaxy's structure looks generally undisturbed. There appears to be no prominent dust lane or significant areas of extinction are visible. The light appears relatively smooth, although there could be a feature present.
