The galaxy presents as a somewhat elliptical, disk-like structure, appearing relatively smooth with a high degree of central concentration. The light distribution appears to be centrally concentrated within the galaxy's body. There appears to be a faint yellowish bulge region that could indicate an aging stellar population, and some blueish, clumpy regions towards one side, potentially indicating ongoing star formation. The galaxy is elongated, with the major axis showing a more extended distribution of light, and the image is consistent with the galaxy being relatively isolated. There is a notable absence of strong spiral arm features, leading to the classification of this galaxy as likely early-type with a smooth morphology. A slight asymmetry is apparent with possibly minor disturbances on one side that could imply minor tidal interactions.
