The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The light distribution appears centrally concentrated, with a fairly rapid falloff in intensity moving outwards from the core. The galaxy's overall shape is somewhat elliptical. The color profile is dominated by reddish hues, suggesting an older stellar population. There is a subtle hint of bluer colors in the outer regions, implying the presence of some younger stars but not a substantial amount of ongoing star formation. No distinct spiral arms or bar structures are discernible. There is no indication of any major ongoing merger activity or significant tidal disturbances. The galaxy appears mostly undisturbed.
