The galaxy presents a moderately inclined, disk-like structure with a noticeable central bulge. The light distribution suggests a relatively smooth morphology, exhibiting a somewhat elongated shape reminiscent of a cigar. A subtle but distinct feature may indicate the presence of a minor disturbance in the galaxy's structure, potentially linked to past interactions or internal processes. The galaxy's color gradient indicates an older stellar population with reduced star formation. The galaxy is not a perfect spiral, nor is it perfectly elliptical, placing it somewhere in between along the Hubble Sequence.
