The galaxy presents as a roughly elliptical structure with a concentrated, bright central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population. Extending outward from the core is a fainter, more diffuse disk component. This disk shows some subtle structural features, possibly including faint spiral arms or dust lanes, but overall appears relatively smooth. The galaxy exhibits a slight tilt relative to our line of sight, offering a partial view of the disk structure. There is no strong evidence of ongoing major mergers, although subtle distortions or asymmetries may be present suggesting the possibility of minor interactions or past disturbances. The overall color gradient suggests a radial variation in stellar population, with bluer, younger stars perhaps present within the outer disk regions.
