The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. It lacks the distinct spiral arm structures characteristic of spiral galaxies. The light distribution is concentrated towards the center, displaying a bright, well-defined core that gradually fades outward. There is a noticeable absence of significant dust lanes or prominent features indicative of recent major mergers or disturbances, although the presence of minor disturbances cannot be entirely ruled out. The galaxy exhibits a reddish hue overall, suggesting an older stellar population dominated by evolved stars and a relatively low rate of current star formation. The apparent lack of blue light indicates that the contribution from young, massive stars is minimal.
