The galaxy presents an elliptical morphology, appearing somewhat elongated, almost cigar-shaped. It exhibits a relatively smooth light distribution. A concentrated central bulge is visible, surrounded by a more diffuse halo of light. The color gradient transitions from a yellowish-white core region to a redder periphery, suggesting older stellar populations are present in the outer regions. There is little evidence of distinct spiral arms or active star formation regions from the galaxy's overall smooth appearance. Possible minor distortions are visible in the shape, potentially suggesting a past or ongoing minor interaction, although a larger part of the population estimates the galaxy is undisturbed. The overall appearance suggests that the galaxy is an evolved system.
