The galaxy presents an overall elliptical morphology, with an apparent cigar-shaped elongation. The light distribution is dominated by a smooth, centrally concentrated bulge, exhibiting a yellowish hue indicative of an older stellar population. A fainter, diffuse disk component is suspected, hinted at by the slight extension along the major axis. No distinct spiral arm structures or significant dust lanes are discernible. There appears to be very little active star formation, which is consistent with the color index and smooth morphology.
