The galaxy presents as a dominant, centrally concentrated spheroid with a smooth light profile. This central bulge exhibits a yellow-red hue, suggesting an older stellar population with relatively low ongoing star formation. A faint, disk-like structure appears to extend from the central bulge, slightly elongated in shape. It is bluer than the central region. There is a notable feature of an arc in the galactic halo, likely a remnant of a past tidal interaction with another object. There is no evidence of current mergers with other large galaxies.
