The galaxy presents as a somewhat elliptical structure, elongated along a roughly horizontal axis in the image frame. The light is concentrated towards the center, exhibiting a bright central bulge. The color profile transitions from a yellow-orange core to slightly bluer hues towards the peripheral regions, particularly noticeable on the left side. There is a subtle irregularity or extension on the left side of the galaxy, possibly indicating some form of tidal interaction or recent accretion event. The overall smooth appearance and dominant central bulge suggest a classification leaning towards an early-type spiral or an elliptical galaxy. However, the slight blue color and extension on the left side implies a possible small amount of on-going star formation. There are no obvious signs of major ongoing merger activity, though minor disturbances cannot be ruled out.
