The galaxy exhibits a somewhat elongated, cigar-shaped morphology. It presents a generally smooth appearance, with little evidence of significant, large-scale features such as spiral arms or prominent dust lanes. A central, bright region is visible, likely a galactic bulge. A faint disk surrounds the bulge. The color distribution suggests a relatively uniform stellar population, possibly with older stars dominating its structure. There are no obvious signs of a major merger event, but a subtle irregularity in the overall shape could hint at a minor interaction or disturbance. The galaxy's disk is oriented close to edge-on relative to our line of sight, giving it the observed elongated shape. The galaxy has a noticeable red-shift, indicating it is moderately distant.
