The galaxy appears to be an elliptical galaxy, cigar-shaped in projection, with a smooth overall morphology. The color suggests an older stellar population. There is a bright, concentrated central bulge region that transitions smoothly into a surrounding halo of decreasing surface brightness. The absence of defined spiral arms or significant dust lanes supports the elliptical classification. There may be faint signs of a minor tidal disturbance or faint feature emanating from the galaxy, but this is uncertain. The galaxy exhibits a red color with faint blue regions in the disk, suggesting some ongoing star formation. The galaxy is relatively isolated, with no apparent nearby companions or interacting features.
