The galaxy presents as an elongated structure, likely a flattened spheroid viewed at an oblique angle. A bright central bulge dominates the core region, exhibiting a concentrated luminosity. The outer regions of the galaxy appear fainter and more diffuse, transitioning into a less defined halo. The color profile suggests a mix of stellar populations, with a bluer hue possibly indicating regions of ongoing star formation. The overall morphology leans towards a smooth, featureless appearance. Subtle irregularities in the outer regions could be indicative of minor gravitational interactions or internal disturbances. The galaxy displays a general lack of prominent spiral arm structures or distinct dust lanes. Its shape is more akin to a cigar shape, with no clearly defined spiral arms. No major ongoing merger events are visible.