The galaxy presents an elongated, somewhat cigar-shaped morphology. The central region exhibits a higher surface brightness, suggesting a concentrated stellar population or an active galactic nucleus. Extending outwards from this central bulge, there appear to be faint, diffuse features, potentially indicative of spiral arms or tidal debris. There is a notable lack of distinct, well-defined spiral arm structures, leading to a classification leaning towards a lenticular or possibly an irregular galaxy. The color gradient across the galaxy is subtle but discernible, with a slightly bluer hue in the outer regions compared to the central area. This may point to ongoing star formation activity in the outskirts. There appears to be some disturbance in its overall form, perhaps resulting from a minor gravitational interaction or past merger event. The galaxy's overall structure suggests it is at an intermediate redshift, and its physical size is relatively substantial. Overall, it is a relatively luminous and massive object.
