The object appears to be a relatively small galaxy, approximately 2.5 kpc in effective radius. Its morphology is generally smooth and rounded, lacking distinct spiral arms or a prominent disk structure. It appears fairly uniform in color, with a slightly enhanced intensity in the central region, suggesting a possible core. The lack of distinct features points towards a galaxy that may be an elliptical or lenticular type, potentially an early-type galaxy that has largely exhausted its supply of gas for star formation. There is no obvious signs of recent merger activity or significant tidal disturbances that could be visually detected. The light is mostly faint red, with very little blue, suggesting a population of older stars. The galaxy shows no evidence of a recent merger or strong interactions, appearing to be in a relatively isolated state.
