The galaxy presents as an elliptical morphology, appearing generally smooth and centrally concentrated with a notable lack of distinct spiral arm structures. It exhibits an elongated shape, being moderately cigar-shaped, and lacks any significant signs of ongoing major merger activity or strong tidal disturbances in the surrounding region. The color profile indicates a relatively evolved stellar population, showing a yellowish hue in its central region that transitions to a bluish color in the outer regions of the disk. This implies the presence of some level of star formation, albeit at a relatively low rate. Overall, the galaxy seems to be an evolved system exhibiting a smooth profile.