The galaxy appears as a centrally concentrated object with a largely smooth morphology. There is little evidence of spiral arm structure or a prominent disk. The light profile gradually fades from a bright, yellowish core outwards to a diffuse, bluish halo. The overall shape is roughly elliptical, appearing neither perfectly round nor highly elongated. The color gradient suggests a possible difference in stellar populations, with the central region potentially dominated by older, redder stars, and the outer regions exhibiting a bluer hue, perhaps indicating the presence of younger stars or ongoing star formation. There is no clear indication of any major ongoing merger events or significant tidal disturbances within the visible structure of the galaxy, though subtle asymmetries might indicate a past interaction.
