The observed galaxy appears as a fairly compact object with a generally smooth morphology. The galaxy exhibits an elliptical shape. The light distribution is somewhat concentrated towards the center, suggesting a high degree of central mass concentration. There are hints of some internal structure, but no clear spiral arms or bars are visible. The galaxy's color suggests an older stellar population, with a redder hue dominating the observed light. There's no significant evidence of ongoing major merging activity. Minor disturbances or tidal features might be present but are not prominently visible.
