The galaxy presents as an elliptical morphology, exhibiting a generally smooth, centrally concentrated light distribution. The core region displays a bright, yellowish-orange hue, suggesting an older stellar population. The galaxy appears fairly symmetrical with no obvious spiral arms or prominent disk features. The overall color index indicates a population dominated by evolved stars, with low levels of ongoing star formation. There is no significant tidal distortion or evidence of a major merger event readily visible. The galaxy has a round shape and the overall structure implies a relatively relaxed dynamical state. The size appears to be intermediate in relation to other galaxies observed within the field of view.
