This galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a smooth, elongated profile. It is observed at an angle, appearing as a cigar shape. The central bulge displays a concentrated luminosity with a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a faint, relatively smooth disk component. The bluer colors in the disk indicate the presence of some younger stars, even though the star formation rate appears to be relatively low. There are no prominent spiral arms or dust lanes visible. The galaxy appears relatively isolated with no signs of ongoing major mergers or significant tidal disturbances.
