The galaxy presents an elliptical morphology, appearing elongated with a high degree of smoothness. There is a concentrated central bulge exhibiting a yellow-red hue, suggesting an older stellar population and potentially lower levels of ongoing star formation. The outer regions appear less defined, fading into the background sky with a bluer tint. The overall structure does not show any strong signs of recent or ongoing major mergers or significant tidal disturbances. There are no prominent spiral arms visible, further supporting the classification as an elliptical type galaxy. The observed color gradient, with the core being redder than the outer regions, could be due to differences in stellar populations or dust distribution. The object’s smooth and somewhat cigar-like shape also hints at an elliptical classification.
