The galaxy appears as a roughly elliptical, luminous structure. The central region exhibits a significantly higher surface brightness, suggestive of a prominent galactic nucleus or bulge. Moving outwards from the center, the luminosity gradually decreases, transitioning into a fainter, less defined halo. The color profile indicates a yellowish-red hue, which, when combined with its morphology, implies an older stellar population. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. The galaxy appears relatively isolated, without clear signs of major tidal disruption or ongoing merger activity, though the shape is slightly elongated and could indicate minor past interactions.
