The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The shape is generally round.

The galaxy exhibits a color gradient, with a yellowish or slightly reddish hue towards the core, suggesting an older stellar population and a higher concentration of dust in the central regions. The outer regions appear slightly bluer, hinting at the presence of younger, hotter stars but their presence is minimal. There is no clear evidence of ongoing major merging activity or tidal disturbances.
