The galaxy presents as a relatively smooth, centrally concentrated structure with a generally elliptical morphology. There is a slight elongation visible, suggesting a deviation from a perfectly circular form. The color profile indicates a redder overall hue, indicative of an older stellar population and/or significant dust obscuration. There is little evidence of prominent spiral arms or active star-forming regions. The galaxy exhibits a fairly uniform surface brightness, lacking any clear, distinct features or intense knots of light. The galaxy appears undisturbed, showing no obvious signs of major tidal interactions or ongoing mergers. There may be a faint hint of asymmetry, but this requires further investigation to ascertain if it is an intrinsic feature or a result of observational noise.