The galaxy exhibits a morphology that is generally smooth, with a slight elongation in its shape. It appears more rounded than cigar-shaped. The central region displays a concentrated, bright core that fades into the outer regions. The color profile suggests a population of older stars dominating its composition, with a redder hue overall. There may be a presence of a minor disturbance in the structure, however it is difficult to confirm given the overall appearance. From what can be observed, the galaxy does not show a clear presence of a significant amount of active star formation.
