The galaxy presents as a relatively smooth, centralized object with a slightly elliptical morphology. The color profile suggests the presence of both older stellar populations, indicated by the reddish hues, and regions of ongoing or recent star formation, as evidenced by the bluer tones. There is faint evidence of some minor disturbances in the overall light distribution, potentially suggesting minor tidal interactions or past merger events. The galaxy does not appear to be undergoing a major merger or exhibit strong tidal features. The concentration of light is quite high at its center, with the light diminishing gradually outwards. The diameter of the galaxy appears to be approximately 9-10 kpc, placing it in the size range of a typical spiral galaxy.
