The galaxy presents a generally smooth morphology, with a somewhat rounded appearance. There is a subtle elongation present, but no distinct spiral arms or bar structures are discernible. The light distribution appears relatively uniform across the galaxy's body, suggesting an older stellar population. A slight color gradient is observed, transitioning from a more yellowish hue at the core to a redder tint toward the outer regions. The overall structure indicates that it's likely a galaxy with little to no active star formation. There seems to be evidence of a possible minor disturbance or interaction, but it is not immediately clear if this is due to a merger or tidal effects from a neighboring galaxy.
