The galaxy presents as an elongated, cigar-shaped structure, generally smooth in appearance, with a distinct central bulge. A faint, disk-like feature is observable, presenting a greenish hue, potentially indicating ongoing star formation. The color gradient suggests an older stellar population dominating the central region, shifting towards younger, star-forming regions in the apparent disk. A subtle disturbance may be present on one side of the galaxy, though no significant signs of ongoing merger activity are immediately apparent. The galaxy exhibits a color profile suggesting moderate to high mass and low specific star formation rate.
