The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and concentrated light profile. There is no apparent spiral arm structure or significant dust lane obscuration visible at this resolution. The overall color is yellowish, suggestive of an older stellar population with a relatively low rate of ongoing star formation. Some slight asymmetry in the galaxy's light distribution hints at possible minor disturbances, potentially indicating past interactions or accretion events, although no clear signs of tidal tails or merging features are immediately apparent. The galaxy appears relatively isolated, with no obvious companion galaxies in close proximity within this field of view.
