The galaxy presents a concentrated, relatively smooth morphology. The central region exhibits a bright, yellowish hue, indicative of an older stellar population and possibly dust obscuration. Moving outwards, the galaxy gradually fades into the surrounding space, with a subtle transition in color toward redder tones in the outskirts. There's a slight elongation apparent, suggesting it may not be perfectly spherical, tending towards a more elliptical shape. The overall structure appears largely undisturbed, with no obvious signs of major tidal interactions or prominent spiral arms. Possible minor disturbances, such as subtle asymmetries or faint plumes, may be present upon closer inspection. The galaxy appears as a single, relatively isolated object.
