The galaxy appears to be a relatively luminous, disk-shaped galaxy exhibiting a moderately inclined orientation relative to our line of sight. Its overall morphology suggests characteristics somewhere between lenticular and spiral, with a smooth, centrally concentrated bulge and a discernible, though somewhat ill-defined, disk. The color gradient suggests an older stellar population, with a yellowish-white bulge indicative of evolved stars and a slightly bluer disk, hinting at ongoing, but potentially subdued, star formation activity. There is no obvious presence of distinct spiral arms. The galaxy's profile is elongated, with an axial ratio indicating a mild degree of ellipticity. There appear to be hints of tidal distortions within the galaxy.
