The galaxy appears as a single, centrally concentrated object, showing a high degree of smoothness. The light profile seems fairly uniform, lacking any distinct spiral arms or a prominent central bar. The galaxy's overall shape is tending towards round, although it does not appear to be perfectly spherical. There are no obvious signs of recent or ongoing major mergers, tidal tails, or other significant disturbances in its morphology. The galaxy exhibits a color gradient, being somewhat bluer in its central regions and becoming redder towards the outer edges. This suggests a possible difference in stellar populations between the center and the outskirts, with younger, hotter stars potentially dominating the core and older, redder stars being more prevalent in the halo. Based on the redder color and lack of any visible blue features, the galaxy is likely composed of older stars and therefore a low amount of star formation. 
