The galaxy presents as a single, centrally concentrated object with a relatively smooth morphology. There is a high degree of central concentration, with the light appearing brightest and most intense at the core, gradually decreasing in intensity outwards. 

The galaxy exhibits a primarily elliptical shape, with a slight deviation towards an intermediate form rather than a perfectly round configuration. There are subtle hints of asymmetry, but no definitive tidal tails or other signs of a major merger are readily apparent. The galaxy shows a color gradient, transitioning from redder hues at the center to greener and eventually bluer shades in the outer regions, suggesting a variation in stellar populations, with older, redder stars dominating the core and younger, bluer stars more prevalent in the periphery.

Given the overall appearance, the galaxy is likely a relatively massive system with a substantial population of older stars and a comparatively low rate of ongoing star formation.
