The galaxy presents as a relatively compact, elliptical-like structure. Its core appears bright and somewhat orange, indicative of an older stellar population. The galaxy's light profile suggests a centrally concentrated mass distribution, with the luminosity decreasing gradually towards the outer regions. There is minimal evidence of spiral arms or a distinct disk. The overall smooth appearance could imply that this is a more evolved galaxy, or one in an early stage of development without well-defined galactic structures. Faint blue tinges around the central region could potentially indicate more recent pockets of star formation, though this activity appears to be limited. There is no clear indication of interaction or merging with another galaxy, and no major disturbances in morphology are immediately apparent.
