The galaxy presents as a generally smooth, elliptical structure with a slightly elongated morphology. The central region exhibits a concentrated luminosity profile, appearing brighter and with a reddish-orange hue. This likely indicates a population of older stars dominating the core. Proceeding outwards from the center, the galactic disc displays a more diffuse and less intense color profile, transitioning towards a subtle blue-green tint. This suggests some presence of younger, hotter stars, possibly within areas of modest star formation activity. There is no strong visual indication of a significant spiral arm structure or a prominent central bulge. There are very subtle signs of asymmetry, suggesting possible minor disturbances or interactions. The galaxy appears relatively isolated, with no obvious major companion galaxies or ongoing major merger events in this field of view.
