The observed galaxy presents a relatively smooth morphology with a faint disk structure. The central bulge appears luminous and somewhat spheroidal, exhibiting a yellowish-white hue, suggesting an older stellar population. The disk component displays a bluer tint, possibly indicative of younger, hotter stars and ongoing star formation. The galaxy is elongated, appearing cigar-shaped, indicating it is observed at an oblique angle relative to its rotational axis. There is a hint of minor disturbances in the outer regions, potentially signs of past or ongoing interactions. The overall color profile suggests a moderate redshift.
