This galaxy presents as a disk galaxy, viewed almost edge-on. There is a distinct central bulge region with a yellowish hue, suggesting a population of older stars. The disk exhibits a relatively smooth structure, with a subtle gradient in color from the central bulge towards the outer edges. The outer regions of the disk appear fainter and bluer, possibly indicating ongoing star formation. No prominent spiral arms are visible. There are subtle signs of minor irregularities or disturbances along the disk, perhaps indicating minor gravitational interactions or recent accretion events. The galaxy appears relatively isolated with no obvious signs of a major ongoing merger or significant tidal disruption. The elongated morphology suggests a high inclination angle relative to our line of sight.
