The galaxy presents as an elongated, ellipsoidal structure. It exhibits a centrally concentrated bulge, characterized by a smooth, diffuse light distribution, yellow in color. Moving outward from the core, there is a subtle transition to a more extended disk-like component. This outer region appears less structured and the color shifts towards the redder part of the spectrum. The color could indicate the presence of an older stellar population. There's no readily apparent evidence of spiral arms or strong star-forming regions. The galaxy's overall morphology indicates an intermediate inclination angle relative to our line of sight. There is no evidence of tidal tails or disrupted features, suggesting that it has not undergone any major merger events recently.
