This galaxy exhibits a relatively smooth morphology with a slight elongation. The main body of the galaxy presents a concentrated, bright core surrounded by a fainter, more diffuse halo. The color distribution indicates a mix of stellar populations; the central region appears to be dominated by bluer light, potentially indicating ongoing or recent star formation, while the outer regions show a shift towards redder hues, suggesting a population of older stars. There may be some minor disturbances in the morphology, but overall the galaxy does not show strong evidence of a major merger or significant tidal interactions. The overall structure suggests a disk-like morphology, with the possibility of a slight bar feature running through the center.
