The galaxy presents as a relatively compact, elliptical-like object. There is a smooth, centrally concentrated light distribution, with a notable lack of spiral arm structure or prominent dust lanes. The color profile suggests an older stellar population, dominated by reddish hues in the core and with some bluer stars in the outskirts, indicating ongoing star formation. The galaxy appears largely undisturbed, without signs of major tidal interactions or ongoing mergers, although there may be a slight asymmetry in the outer halo. The object exhibits moderate luminosity. The overall morphology points towards a relatively evolved system, potentially transitioning from a spiral-like to an elliptical-like form.
