The galaxy presents as a moderately inclined, disk-shaped structure. It appears relatively smooth with no distinct spiral arms. The color profile is predominantly reddish-orange, indicating an older stellar population. The galaxy's morphology suggests a system with an effective radius on the order of several kiloparsecs. The lack of discernible features implies that the disk may be largely devoid of active star formation, consistent with a low specific star formation rate. The elongated, cigar-like shape suggests that it is not perfectly face-on, but rather viewed at an angle, which could be influencing the observed color distribution and smoothing of features. There are no obvious signs of interaction with other galaxies or major tidal disturbances.