The galaxy exhibits a generally smooth morphology, with a subtle disk-like structure. The light distribution appears to be centrally concentrated, with a bright nucleus and a gradual decrease in luminosity outwards. The galaxy's overall shape is elongated, appearing somewhat flattened. The color profile suggests a mix of stellar populations. The central region appears more yellow, potentially indicating the presence of older stars. The outer regions exhibit a slightly bluer tint, which may indicate the presence of younger, hotter stars, and regions of on-going star formation. There is no strong evidence of tidal features or significant disturbances in the galaxy's morphology, which suggest a relative state of equilibrium. The galaxy appears well-defined, without significant signs of recent merger activity.
