The galaxy presents as a luminous, elongated structure, consistent with an elliptical or lenticular morphology viewed at an angle that is not face-on. The central region exhibits a concentrated brightness, suggestive of a significant stellar population and potentially a supermassive black hole nucleus. Progressing outwards from the core, the light intensity decreases gradually. Color gradients are subtle but perceptible. The core appears slightly yellowish, perhaps indicating an older stellar population, while the outer regions exhibit a bluer hue that hints towards ongoing, or recent, star formation. There is a possible minor asymmetry in the light distribution. It is currently unclear if this distortion is a feature of the galaxy's internal structure, or a sign of an external interaction.
