This galaxy appears to be a spiral galaxy viewed at a moderate inclination. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population. The disk is visible but somewhat faint, with hints of spiral arm structure. The disk appears to be a mix of bluer and redder regions, potentially indicating areas of ongoing star formation alongside older stellar populations. The galaxy appears to be relatively isolated, with no obvious signs of tidal interactions or major mergers. It exhibits a generally smooth appearance, with subtle disturbances. Its overall morphology seems to be transitioning between a smooth elliptical form and a more fully developed spiral. The galaxy is elongated, exhibiting a cigar-like shape.
